ライフサイエンスコーパス: intracluster

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1 on an unusual competition between inter- and intracluster bonds.

2 distance between branch points on the short intracluster chains were similar for all genotypes howev

3 Furthermore, changes in intracluster closed time distributions were the single b

4 effective opening rate (increase in the mean intracluster closed time duration) in single-channel rec

5 The intracluster closed-time histograms contained four compo

6 tivation of neural clusters with potentiated intracluster connections, with the firing rate in each c

7 many polymorphisms, consistent with frequent intracluster conversion.

8 nt clusters, analyses of such data must take intracluster correlation into account rather than assumi

9 dds ratios were obtained with correction for intracluster correlation.

10 iptional networks that convey information on intracluster correlations and intercluster connections o

11 The intracluster correlations and the cluster-framework corr

12 l loss with odds ratios, with adjustment for intracluster correlations as appropriate.

13 in Mossbauer spectra, spin ground state, and intracluster Fe-Fe separation.

14 electrons are highly effective at mediating intracluster ferromagnetic exchange coupling between the

15 itting 'bubbles' rising buoyantly in the hot intracluster gas, before later falling back.

16 ting processes (such as shock-heating of the intracluster gas, supernovae, and Active Galactic Nuclei

17 s on the nanocluster form local tetramers by intracluster interactions of C-H...pi and pi...pi stacki

18 nteraction of jets with the intergalactic or intracluster media, and in studying the energy generatio

19 hot (10(7) to 10(8) kelvin), X-ray-emitting intracluster medium (ICM) is the dominant baryonic const

20 s of the interaction between the hot ionized intracluster medium and the cold interstellar medium of

21 Cooling of the hot intracluster medium in cluster centers can feed the supe

22 aboratory experiments, support the idea that intracluster medium turbulence may have significantly co

23 Stars and gas in galaxies, hot intracluster medium, and intergalactic photo-ionized gas

24 is cluster may form through accretion of the intracluster medium, rather than (as is currently though

25 highly compressible low-entropy gas from the intracluster medium.

26 uences with seven other group O isolates (5% intracluster nucleotide sequence diversity) similar to c

27 The intracluster open durations elicited by beta-alanine cou

28 The distributions of the intracluster open durations elicited by GABA could be de

29 concentration of cysteamine that elicits an intracluster open probability of >0.9.

30 The maximal intracluster open probability was 0.35, with a half-maxi

31 e cores of some clusters of galaxies the hot intracluster plasma is dense enough that it should cool

32 Associative intracluster proton transfer Bz(.+)(H2O)(n+1) + H2O-->C6

33 This suggests a barrier to intracluster proton transfer, and as a result, the [Bz(.

34 The intracluster reactions are highly advantageous for appli

35 by sequential addition of HIO3, followed by intracluster restructuring to I2O5 and recycling of wate

36 represent behaviorally distinct stimuli and intracluster variability represents sensory or neuronal

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