ライフサイエンスコーパス: disk

1 density waves in the midplane of this young disk.

2 nto the inner regions of its large accretion disk.

3 ching the inner regions from the rest of the disk.

4 ined mass accretion to the inner part of the disk.

5 modes bounded at the peripheries of a hollow disk.

6 an red blood cell is known to be a biconcave disk.

7 rays from the inner regions of the accretion disk.

8 of the cardiomyocyte and in the intercalated disks.

9 o 1.5 W for ablation of bacteria coating the disks.

10 e biofilm without causing physical damage to disks.

11 section measurements on arrays of gold nano-disks.

12 12 disks and excluded spondylodiskitis in 17 disks.

13 ns in the inner, star-forming regions of the disks.

14 e kill in the biovolume of QAMS-free control disks (3.73 +/- 2.11%) and QAMS-containing experimental

15 +/- 2.11%) and QAMS-containing experimental disks (33.94 +/- 23.88%) retrieved from the subjects (P

16 remove the plaque and TiO2 layer on anodized disks, although both procedures appear capable of restor

17 Ring electrodes consisting of both an inner disk and an outer ring were used to prevent neutral tran

18 only), Streptococcus pneumoniae ATCC 49619 (disk and broth), and Haemophilus influenzae ATCC 49247 (

19 oth), and Haemophilus influenzae ATCC 49247 (disk and broth).

20 The disk and MIC breakpoints evaluated included the Clinical

21 nsis oxacillin MIC breakpoints and cefoxitin disk and MIC breakpoints, the CLSI M100-S25 coagulase-ne

22 Oxacillin and cefoxitin disk and MIC tests were evaluated for the detection of m

23 acillin results interpreted by the VET01-S2 (disk and MIC) and M100-S25 CoNS (MIC) breakpoints agreed

24 We demonstrate high quality (Q) factor ring, disk and photonic crystal resonators using a hybrid sili

25 e formation of Jupiter, opening a gap in the disk and preventing the exchange of material between the

26 h-curvature rim domains of the outer segment disk and suggests that the protein's C terminus may modu

27 associated links, control the sizing of rod disks and cone lamellae throughout their daily renewal.

28 standards identified spondylodiskitis in 12 disks and excluded spondylodiskitis in 17 disks.

29 MacConkey agar plate with a 10-mug meropenem disk) and for sequencing of DNA obtained from carbapenem

30 laser scanning confocal microscopy, spinning disk, and lightsheet microscopy, to study the localizati

31 1.5 is densely expressed at the intercalated disk, and narrow intercellular separation can modulate c

32 ode or select a PDB archive from their local disk, and Web3DMol will display and allow interactive ma

33 a function of the magnetisation state of the disks, and identified a range of different phenomena ari

34 ) versus tryptic soy broth (TSB) to incubate disks, and incubation of plates for 6 h versus 18 to 20

35 eriments with virus particles in tailor-made disk- and annulus-shaped microchambers, that strong conf

36 However, macrocycles were more disk- and spherelike, which may contribute to their supe

37 thode and a liquid drop placed on a graphite disk anode.

38 y, measurements were made on a cross section disk approximately 10cm from the root top at three diffe

39 Two protostars near the centre of the disk are separated by 61 astronomical units and a tertia

40 We demonstrate that the disk around L1448 IRS3B appears susceptible to disk frag

41 sec resolution (12 au) of the protoplanetary disk around V883 Ori, a protostar of 1.3 solar masses th

42 in the binary potential and forms accretion disks around both black holes.

43 places an enormous burden on computational, disk array, and network resources.

44 cally to minimize the burden on networks and disk arrays, create output files that are minimal in siz

45 ing the magnetization states of nanomagnetic disks as state representations of a vortex and single do

46 module 5 of nebulette extends outward from Z-disk-associated desmin filaments toward the center of th

47 is coincident with a spiral arm in the outer disk at a separation of 183 astronomical units.

48 hat water was depleted in the protoplanetary disk at the planet's formation location, but it is uncle

49 snow-line is the region of a protoplanetary disk at which a major volatile, such as water or carbon

50 s were randomly assigned by drawing numbered disks at random from a bag to do a 2 h walk either along

51 But the water snow-line of a protoplanetary disk (at temperatures of more than 100 kelvin) has not h

52 ghtness at two visible wavelengths provide a disk-averaged estimate of its atmospheric aerosol.

53 of the deposit patterns, the formation of a disk being the robust signature of particles rendered hy

54 CoNS) oxacillin MIC breakpoint and cefoxitin disk breakpoint, the CLSI VET01-S2 S. pseudintermedius o

55 sting (EUCAST) S. pseudintermedius cefoxitin disk breakpoint.

56 T01-S2 S. pseudintermedius oxacillin MIC and disk breakpoints, and the European Committee on Antimicr

57 ectronic heat energy deposited on a graphene disk can be transferred to a neighboring nanoisland with

58 .ebi.ac.uk) are continually expanding: total disk capacity increases significantly every year to keep

59 nstability is supposed to occur in the inner disk, causing repetitive patterns of large-amplitude X-r

60 joints, sacroiliac joints, or intervertebral disks (combination trial, 202 participants) and were unr

61 communities developed in uncolonized control disks compared with those that had been pre-colonized),

62 the RDNMR signals from Hall bar and Corbino disk configurations allows us to distinguish the contrib

63 noscale topography (DNA-PAINT) with spinning disk confocal (SDC) hardware to overcome this limitation

64 Multiphoton and spinning disk confocal intravital microscopy revealed that monocy

65 Using spinning-disk confocal intravital microscopy to track MRSA-GFP in

66 By using spinning-disk confocal intravital microscopy, we examined the mol

67 opment of a cryo-stage allowing for spinning-disk confocal light microscopy at cryogenic temperatures

68 Spinning disk confocal microscopy and 3D reconstruction revealed

69 We use spinning-disk confocal microscopy to capture 3D volumetric fluore

70 Using spinning disk confocal microscopy to image filopodial dynamics in

71 Using live-cell spinning disk confocal microscopy, we measured the motility of ce

72 Using spinning disk confocal microscopy, we observe fast fluctuations o

73 This disk contains four Apaf-1/pc-9 CARD pairs arranged in a

74 on volts), which is ascribed to an accretion disk corona of energetic particles akin to those seen in

75 iquity, the physical conditions in accretion disk coronae remain poorly constrained.

76 , the Chemcatcher containing an Atlantic HLB disk covered by a 0.2 mum poly(ether sulfone) membrane,

77 e array of micrometer-sized Py ferromagnetic disks covered by a superconducting Nb thin film.

78 nostructured morphologies including spheres, disks, cylinders, and vesicles.

79 with chronic back pain diagnosed with lumbar disk degeneration and unresponsive to conservative treat

80 ing to the emission from the inner accretion disk demonstrates a connection between accretion process

81 al agreement were highest for fluconazole by disk diffusion (0.902, standard error [SE] = 0.076) and

82 (1.00, SE = 0.218) and for amphotericin B by disk diffusion (1.00, SE = 0.098).

83 s for a fixed tazobactam MIC of 8 mug/ml and disk diffusion (30/20-mug disk) test methods were approv

84 . pneumoniae, and 15 S. pyogenes isolates by disk diffusion (DD) methods.

85 1 (1%) major and 5 (4.8%) minor errors with disk diffusion and 4 (13.3%) minor errors with Etest.

86 sceptibilities from blood culture bottles by disk diffusion and Etest and the results of standardized

87 rly into agar, potentially giving inaccurate disk diffusion and Etest results.

88 All disk diffusion and MIC QC ranges established in this stu

89 Disk diffusion and MIC quality control (QC) ranges were

90 ontrol (QC) study was performed to establish disk diffusion and MIC ranges for cefepime-tazobactam fo

91 The cefoxitin disk diffusion and oxacillin broth microdilution assays

92 Thus, antifungal disk diffusion directly from blood culture bottles is a

93 This multicenter study evaluated cefoxitin disk diffusion for 37 atypical S. aureus isolates (156 r

94 (-0.42) precludes the use of amphotericin B disk diffusion for susceptibility testing.

95 tibility test was done using the Kirby-Bauer Disk diffusion method according to the guidelines of Cli

96 usceptibility to 11 antimicrobials using the disk diffusion method and validated using VITEK 2 (bioMe

97 With the disk diffusion method using MH agar from BD and Oxoid, s

98 microbial activity was evaluated by the agar disk diffusion method, and in vitro cytotoxic activity w

99 Nafithromycin disk diffusion QC ranges were determined to be 25 to 31

100 Additionally, a cefoxitin disk diffusion test and an oxacillin broth microdilution

101 cy of penicillin MIC testing, the penicillin disk diffusion test, and three beta-lactamase tests, inc

102 Disk diffusion testing of fosfomycin was performed on 64

103 in antimicrobial susceptibility testing from disk diffusion to an automated susceptibility testing sy

104 al agreement with blaZ PCR, while penicillin disk diffusion yielded one major error.

105 a, we evaluated the performances of Vitek 2, disk diffusion, and a MicroScan panel compared to that o

106 n clinical microbiology laboratories (Etest, disk diffusion, and Sensititre broth microdilution metho

107 and Acinetobacter baumannii through in vitro disk diffusion, broth dilution and time-kill studies.

108 ttery of confirmatory testing which included disk diffusion, Microscan broth microdilution, Clinical

109 with alternative phenotypic testing methods (disk diffusion, Microscan broth microdilution, CLSI brot

110 and amphotericin B susceptibility results by disk diffusion.

111 included hypertension, asthma, degenerative disk disease, and migraine, all of which were reportedly

112 xcite spiral density waves in protoplanetary disks, disks of gas and dust orbiting young stars.

113 Rod basal outer disks displayed excessive outgrowth, and cone outer segm

114 o parallel line patterns on the surface of a disk drive medium.

115 ce inside a commercial magnetic storage hard disk drive provides a unique system for such studies.

116 al scanner, comprising a LightScribe compact disk drive, was developed to measure the diffraction pat

117 asure the magnetic field generated by a hard-disk-drive write head with high spatial resolution and l

118 cale fragmentation of a massive protostellar disk due to gravitational instability.

119 The self-assembled monolayer protected gold-disk electrode (AuDE) was coated with a reduced graphene

120 A dip-type small diameter ring-disk electrode (RDE) is ideal for very small volumes.

121 DNA (ss-HSDNA/rGOae) modified on a rotating disk electrode (RDE) is presented.

122 assical Koutecky-Levich model for a rotating disk electrode (RDE) to a general heterogeneous electroc

123 mic diffusion of the ss-HSDNA/rGOae rotating disk electrode (RDE) toward AFB1 detection using FcCH2OH

124 electrochemical study by using rotating ring disk electrode (RRDE) methods over a wide potential rang

125 Rotating disk electrode and rotating ring disk electrode studies

126 l mass transfer resistances using a rotating disk electrode exhibited only a 5% reduction in current,

127 d using cyclic voltammetry and rotating ring-disk electrode method.

128 Rotating disk electrode and rotating ring disk electrode studies of the polydopamine-coated materi

129 Rotating ring-disk electrode studies were completed to probe the Farad

130 es of hydrodynamic SECM imaging of a 2 mm Pt disk electrode surface in the SG/TC mode based on in sit

131 This study utilized the rotating ring-disk electrode technique to examine the reduction kineti

132 ons as cyclic voltammogram and rotating ring-disk electrode tests show that the potential of oxygen r

133 n in neutral aqueous solutions at a rotating disk electrode to be oxidized at a concentric Au ring el

134 ticles drop-coated on glassy carbon rotating disk electrode using Nafion as a binder.

135 yses, scanning electron microscopy, rotating disk electrode voltammetry, demonstrate that Li2O2 elect

136 ed in which the potential of a glassy carbon disk electrode was linearly scanned in the oxygen reduct

137 experiments with a commercial rotating ring disk electrode.

138 ecular recognition elements (MREs) onto gold disk electrodes (GDEs).

139 Rotating disk electrodes (RDEs) are widely used in electrochemica

140 Two models based on rotating disk electrodes and flow chronopotentiometry at metal-ba

141 onized material, expelled from the accretion disk encircling the black hole, and collimated radio jet

142 e result is inconsistent with the low-energy disk equilibration model, but supports the high-energy,

143 netic fields by writer pole of magnetic hard disks, especially for achieving increased areal density

144 must be considered when developing models of disk evolution and planet formation.

145 Snow-lines play a crucial role in disk evolution by promoting the rapid growth of ice-cove

146 ning potential when the magnetisation of the disks evolves from the vortex-like state to an onion-lik

147 At remanence the disks exist in almost fully flux-closed magnetic vortex

148 talysis (kobs) determined from rotating ring-disk experiments (1.1 vs 0.05 h(-1)) establish a cofacia

149 system with which to search for evidence of disk fragmentation as it is in an early phase of the sta

150 sk around L1448 IRS3B appears susceptible to disk fragmentation at radii between 150 and 320 astronom

151 Previous evidence for disk fragmentation was limited to inferences based on th

152 meteorites and, by inference, the primordial disk from which they formed.

153 o be a fast-spinning, rotationally supported disk galaxy.

154 ter Solar System, possibly by the opening of disk gaps from the early formation of gas giants.

155 While the glass fiber filter disk has a higher capture efficiency ( approximately 40%

156 or dozens of kiloparsecs beyond the galactic disks-host an active nucleus, and two of them also have

157 creted from an equatorial circum-terrestrial disk; however, the current lunar orbital inclination of

158 lations, because the outer part of the large disk in binaries with long orbital periods will have sur

159 were applied to the surface of sound dentin disks in 4 experimental groups: non-antibacterial adhesi

160 ting of Pg strain 381 were grown on titanium disks, including: 1) sandblasted, large-grit, acid-etche

161 e, the mass of dark matter within a galactic disk increases with disk radius, becoming appreciable an

162 gar plates (BAP), with and without cefoxitin disk induction.

163 covery sequences; reference for ligament and disk injuries and contusion or occult fracture) for trau

164 of carry-across effect and allocation bias (disks inserted in the left or right side of retainer), s

165 ch lower mass-transfer rates, when accretion-disk instabilities drop matter onto the white dwarfs.

166 ot the critical parameter for inducing inner-disk instabilities.

167 Here, we demonstrate that head-disk interface inside a commercial magnetic storage hard

168 Here, we have used multilaser spinning-disk intravital microscopy to monitor the blood-borne st

169 e large velocity dispersion in high-redshift disks introduces a substantial pressure term that leads

170 table anchoring of titin within the muscle Z-disk is essential for preserving muscle integrity during

171 During activation an acentric disk is formed on the central hub of the apoptosome.

172 the zone of inhibition around the fosfomycin disk is occasionally observed upon susceptibility testin

173 main candidates for anchoring titin in the Z-disk is the actin cross-linker alpha-actinin.

174 f PN-1 in the pathogenesis of intervertebral disk (IVD) degeneration.

175 The micro-disk laser has been fabricated by means of a combination

176 nd obtained its gaseous envelope late in its disk lifetime, with little contamination from metal-rich

177 he kinetochore is often depicted as having a disk-like architecture in which the outer layer of prote

178 Illustrated with disk-like C-S-H building blocks, this study provides a d

179 spect ratio (diameter-to-thickness ratio) of disk-like C-S-H building blocks.

180 in the absence of Cl(-), only isotropic and disk-like Cu2-xS nanocrystals form.

181 t, very compliant spheres naturally assume a disk-like geometry and dynamic orientation that are favo

182 The disk-like planar supports are usually prepared by sequen

183 long hydrophobic grooves that run around its disk-like shape to recognize and bind to multiple hydrop

184 tric including pushpin-, star- and biconcave disk-like structures, as well as more complex jellyfish-

185 Experimental disks made of titanium (Ti) or zirconia (ZrO2) with a ma

186 ferences in gepotidacin disk results between disk manufacturers and some agar types and also with pot

187 ce of magnetically gated accretion, in which disk material builds up around the magnetospheric bounda

188 high-curvature rim domains of outer segment disk membranes suggests that it may act to shape these s

189 psin, may indeed exist as a homodimer in rod disk membranes.

190 ted to be the sole species present in native disk membranes.

191 ed for ESBL production using the combination disk method and confirmed using VITEK 2.

192 from conventional biochemical and cefoxitin disk methods performed at an independent laboratory.

193 rm between a counter electrode and a working disk microelectrode.

194 When tracked by TIRF and spinning-disk microscopy, cells expressing phosphomimicking Cav1

195 owed spiral structure were not able to probe disk midplanes, where most of the mass is concentrated a

196 predict the degree of polymerization (DP) of disk-milled fibrils using CHFX and milling time or milli

197 ion in producing cellulose nanofibrils using disk milling with substantial mechanical energy savings.

198 (GARPs) are required for phototransduction, disk morphogenesis, and rod structural integrity.

199 The inclusions are silicon disk nanoantennas embedded in a flexible supporting laye

200 The plasma composition in full-disk observations of the Sun is related to the evolution

201 obing the microwave response of a magnetised disk of Cr-(Bi,Sb)2Te3.

202 In both types of links, opaque disks of different sizes are used to obstruct the beams

203 piral density waves in protoplanetary disks, disks of gas and dust orbiting young stars.

204 e hair cell stereocilia and the intercalated disks of isolated cardiac myocytes, and performed target

205 as a function of disk radius) for the outer disks of six massive star-forming galaxies, and find tha

206 minant in the outer, baryonic regions of the disks of star-forming galaxies.

207 cluding adhesion plaques and dense bodies (Z-disks) of striated muscles and attachment plaques of smo

208 re tested: Staphylococcus aureus ATCC 25923 (disk only), S. aureus ATCC 29213 (broth only), Enterococ

209 d that laboratories should perform oxacillin disk or MIC tests of these isolates when they are encoun

210 The arms extend to the disk outer regions and can be traced down to the midplan

211 .056), longitudinal ligaments (P = .412), or disk (P = .665) injuries.

212 2 enrich at the same region of the chromatin disk periphery during this window of cell division and t

213 The arrangement of the graphite disk placed on a PTFE chip platform as well as the solid

214 joints, sacroiliac joints, or intervertebral disks, radiofrequency denervation combined with a standa

215 (showing rotation velocity as a function of disk radius) for the outer disks of six massive star-for

216 matter within a galactic disk increases with disk radius, becoming appreciable and then dominant in t

217 he disk that are constant or increasing with disk radius-a hallmark of the dark-matter model.

218 Its stars must have formed in a disk, rather than in a merger-driven nuclear starburst.

219 SUV ratios (affected disk/reference disk) were determined.

220 We demonstrate that for disk resonators on low-index quartz substrates, the elec

221 al and numerical characterization of Silicon disk resonators.

222 (respectively charged) residues can lead to disk (respectively ring) deposit morphologies independen

223 also some slight differences in gepotidacin disk results between disk manufacturers and some agar ty

224 or all other variations, gepotidacin MIC and disk results were considered comparable to reference res

225 ly, tetramer polymerization, localization at disk rims, interaction with GARP2, or the generation of

226 We showed that the anisotropic disk shape of nanoplasmonic upconverting nanoparticles (

227 cardiopulmonary distress) to either rod- or disk-shape morphology.

228 asters meet at the midplane, they assemble a disk-shaped interaction zone consisting of anti-parallel

229 In this limit, disk-shaped membranes become unstable, instead forming s

230 he coffee-ring effect and the formation of a disk-shaped pattern is primarily associated with particl

231 In particular, larger rod- and disk-shaped PEG NPs show more uptake than smaller ones,

232 monstrate the successful use of spin-vortex, disk-shaped permalloy magnetic particles in a low-freque

233 assive delivery of preexisting vesicles to a disk-shaped region at the equatorial plane precedes a pr

234 For this, a disk-shaped, membrane-enclosed precursor termed the cell

235 h human embryonic stem cells are confined to disk-shaped, submillimeter colonies.

236 Ultrasound-treated disks showed marked surface changes, incomplete removal

237 Here, we discover that a small moving disk, simulating the sweep of a predator cruising overhe

238 other solutions in terms of the run time and disk space required.

239 The SPR disk surface has been modified with octadecanethiol self

240 Disk surface morphology was evaluated by scanning electr

241 esults show confluent Pg biofilm coating all disk surfaces.

242 ganic radicals in the ionized regions of the disk surrounding the Sun during its formation may have t

243 s is approximately one solar mass, while the disk surrounding the three protostars has a total mass o

244 symmetric spiral arms in the protoplanetary disk surrounding the young star Elias 2-27.

245 20 kelvin) have recently been imaged in the disks surrounding the pre-main-sequence stars TW Hydra a

246 eae with high specificity using the standard disk susceptibility test.

247 and noninfected patients and used the double disk synergy test for extended-spectrum beta-lactamase-p

248 cal depth at about 42 au, where the elevated disk temperature approaches the condensation point of wa

249 Air-water cooling kept disk temperature below the critical threshold of 47 degr

250 plus BA), and an aztreonam plus clavulanate disk test (ATM plus CA).

251 est (CLSI), a boronic acid-supplemented CLSI disk test (CLSI plus BA), and an aztreonam plus clavulan

252 signed to compare ESBL detection by the CLSI disk test (CLSI), a boronic acid-supplemented CLSI disk

253 -48 disk test, and high-inoculum [HI] OXA-48 disk test) and a new ICT (OXA-48 K-SeT) were compared by

254 for faropenem, 53.6% and 100% for the OXA-48 disk test, 98.8% and 97.6% for the HI OXA-48 disk test,

255 disk test, 98.8% and 97.6% for the HI OXA-48 disk test, and 100% and 100% for the ICT, respectively.

256 illin disk test, faropenem disk test, OXA-48 disk test, and high-inoculum [HI] OXA-48 disk test) and

257 Four phenotypic tests (temocillin disk test, faropenem disk test, OXA-48 disk test, and hi

258 typic tests (temocillin disk test, faropenem disk test, OXA-48 disk test, and high-inoculum [HI] OXA-

259 IC of 8 mug/ml and disk diffusion (30/20-mug disk) test methods were approved by the CLSI Subcommitte

260 Ball-on-disk tests at contact pressures of 1.3 gigapascals revea

261 Macroscale reciprocating pin-on-disk tests were conducted to assess wear behavior under

262 velocities of the visible matter within the disk that are constant or increasing with disk radius-a

263 is consistent with models for a protostellar disk that has recently undergone gravitational instabili

264 Here, beech (Fagus sylvatica) wood disks that had been pre-colonized with three wood decay

265 r is absorbed into black holes via accretion disks, the state of which depends primarily on the mass-

266 and the small sizes of their protoplanetary disks, there should be a large but hitherto undetected p

267 had orbited in their host galaxies' gaseous disks throughout the period between their initial format

268 ectively) under no-till (NT) or conventional disk tillage (CT) with full irrigation (n = 4).

269 marginal band coiling that occurs during the disk-to-sphere transition observed, for instance, at the

270 al coherence tomography (SS-OCT) and Placido disk topography in eyes with cataracts.

271 ended when a sizeable fraction of the outer disk was depleted by the wind, detaching the inner regio

272 traditional localization at the intercalated disk was preserved.

273 ion of Saos-2 osteoblasts on new and treated disks were assayed by propidium iodide/DNA stain assay a

274 te implant decontamination, the contaminated disks were burnished with 0.12% chlorhexidine, 20% citri

275 Grit-blasted acid-etched titanium disks were contaminated with multispecies microcosm biof

276 y ECs in a static culture, where the smaller disks were found to be uptaken the most.

277 Glass-ceramic disks were immersed in each pH solution for 3 d, then cy

278 PTFOS disks were implanted in two mice; after 30 days, the tis

279 Two control QAMS-free acrylic disks were inserted into the wells on one side of an ort

280 and two experimental QAMS-containing acrylic disks were inserted into the wells on the other side of

281 After 48 hours, the disks were retrieved and examined for microbial vitality

282 SUV ratios (affected disk/reference disk) were determined.

283 revealed a diminished localization at the z disk, whereas traditional localization at the intercalat

284 plied for bacterial adhesion to each type of disk, which after 72 hours of incubation was assessed us

285 r of S, Se, Te and Sb within the proto-lunar disk, which is as of yet virtually unconstrained.

286 ders consisting of hydrogen-bonded G-quartet disks, which are stacked on top of one another.

287 ational radii of the black hole ionizing the disk wind hundreds of gravitational radii further away a

288 observations of a sustained outer accretion disk wind in V404 Cyg, which is unlike any seen hitherto

289 That this disk wind is responding to the emission from the inner a

290 ativistic (that is, near the speed of light) disk winds a few hundred gravitational radii from the bl

291 Gas outflows (in the form of disk winds) release huge quantities of energy into the i

292 ust and molecular gas emission that reveal a disk with a spiral structure surrounding the three proto

293 been achieved using an InGaN/GaN based micro-disk with an undercut structure on a silicon substrate.

294 Subgingival plaque-coated titanium disks with a moderately rough surface were fixed with et

295 from single-component chiral rods form flat disks with uniform edge twist.

296 by passing air through a glass fiber filter disk within a disposable paper spray cartridge.

297 ted as planetesimals from the protoplanetary disk, would constrain a critical phase of planetary form

298 Gepotidacin AD MIC levels were increased and disk zone diameters were decreased for all species in 10

299 the blaZ PCR results, whereas the penicillin disk zone edge and cloverleaf tests showed sensitivities

300 penicillin cloverleaf assay, and penicillin disk zone edge test.