Results 31 to 40 of about 2,712 (226)

Intracluster Medium Abundances Revisited

, 1998
5 pages, 2 figures, LaTeX, requires paspconf.sty, also available at http://msowww.anu.edu.au/~gibson/publications.html, to appear in Abundance Profiles: Diagnostic Tools for Galaxy History, eds D.
Gibson, Brad K., Woolaston, Emma J.
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NGC 7421: Surfing the Intracluster Medium? [PDF]

Publications of the Astronomical Society of Australia, 1997
AbstractNGC 7421 is a barred spiral that is displaced from the centre of its optical envelope, and has a ‘bow-shock’-like western boundary, both suggestive of interaction with an intracluster medium. We have used five configurations of the ATCA to map the distribution and kinematics of HI in NGC 7421, and find supportive evidence for this scenario in ...
Stuart D. Ryder, G. Purcell, D. Davis, V. Andersen   +3 more
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Enrichment of the Hot Intracluster Medium: Numerical Simulations [PDF]

Space Science Reviews, 2018
The distribution of chemical elements in the hot intracluster medium (ICM) retains valuable information about the enrichment and star formation histories of galaxy clusters, and on the feedback and dynamical processes driving the evolution of the cosmic baryons.
Biffi, V., Mernier, F., Medvedev, P.
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Power spectrum estimation methods on intracluster medium surface brightness fluctuations [PDF]

EPJ Web of Conferences
Accurate estimation of galaxy cluster masses is a central problem in cosmology. Turbulence is believed to introduce significant deviations from the hydrostatic mass estimates.
Bishop M., Perrott Y., Parashar T., Oughton S.   +3 more
doaj   +1 more source

The Intracluster Medium inz > 1 Galaxy Clusters [PDF]

The Astrophysical Journal, 2001
4 pages in emulateapj style plus 2 color jpegs for Figure 3.
Stanford SA, Holden B, ROSATI, Piero, Tozzi P, Borgani S, Eisenhardt PR, Spinrad H.   +6 more
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Heating of the intracluster medium

The Astrophysical Journal, 1990
The gravitational interaction of the system of galaxies and the ICM are treated by fluctuation theory. Fluctuation theory seems to be more adequate to describe the gravitational interaction than local theories used up to now, because gravitation is a long-range force.
A. Just, B. M. Deiss, W. H. Kegel, H. Boehringer, G. E. Morfill   +4 more
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Heating and enriching the intracluster medium [PDF]

Monthly Notices of the Royal Astronomical Society, 2012
23 pages, accepted by MNRAS. Some changes in response to referee's comments.
Short, C. J., Thomas, P. A., Young, O. E.   +2 more
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Detrending Changes the Temporal Dynamics of a Semantic Fluency Task

Frontiers in Aging Neuroscience, 2016
Objective: To study the dynamics of clustering semantic fluency responses and switching between clusters. Methods: We conducted a cross-sectional study of participants (N=60) in a study of patient reported outcomes who were given the Saint Louis ...
Steven Lenio, Frances M. Lissemore, Martha Sajatovic, Kathleen Smyth, Curtis Tatsuoka, Wojbor A. Woyczynski, Alan J. Lerner   +6 more
doaj   +1 more source

Deep Synoptic Array Science: Two Fast Radio Burst Sources in Massive Galaxy Clusters

The Astrophysical Journal Letters, 2023
The hot gas that constitutes the intracluster medium (ICM) has been studied at X-ray and millimeter/submillimeter wavelengths (Sunyaev–Zel’dovich effect) for decades.
Liam Connor, Vikram Ravi, Morgan Catha, Ge Chen, Jakob T. Faber, James W. Lamb, Gregg Hallinan, Charlie Harnach, Greg Hellbourg, Rick Hobbs, David Hodge, Mark Hodges, Casey Law, Paul Rasmussen, Jack Sayers, Kritti Sharma, Myles B. Sherman, Jun Shi, Dana Simard, Jean Somalwar, Reynier Squillace, Sander Weinreb, David P. Woody, Nitika Yadlapalli, The Deep Synoptic Array team   +24 more
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Plasma 2020 - Intracluster Medium Plasmas

, 2019
Galaxy clusters are the largest and most massive bound objects resulting from cosmic hierarchical structure formation. Baryons account for somewhat more than 10% of that mass, with roughly 90% of the baryonic matter distributed throughout the clusters as hot ($T>1$ keV), high-$ $, very weakly collisional plasma; the so-called "intracluster medium" (
Caprioli, Damiano, Brunetti, Gianfranco, Jones, Thomas W., Kang, Hyesung, Kunz, Matthew, Oh, S. Peng, Ryu, Dongsu, Zhuravleva, Irina, Zweibel, Ellen   +8 more
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