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    1. http://hea-www.harvard.edu/~pgreen/SOC/5.html
    ... buoyant bubbles in the hot gas in galaxies and groups as well as in rich clusters ... to explain the absence of cold gas in cluster cores, although they appear to be ... and distributions relative to the mass and hot gas of the cluster environment ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~pgreen/SOC/5.html -- 10.7 Кб -- 01.10.2012
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    2. http://hea-www.harvard.edu/~kim/pap/A754_2003.pdf
    ... of the expected quantities of cool gas in cluster central regions (Peterson et al ... is the boundar y between the hot cluster gas and two cool, galaxy-size dense gas ... map is used for an estimate of the thermal conductivity of the cluster gas ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/A754_2003.pdf -- 240.1 Кб -- 06.12.2010
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    3. SAO Summer Intern Program Projects, 2013
    ... of the hot baryonic gas gas belonging to the colliding sub-clusters is dissipated by ... on the hydrodynamical state of the cluster gas, both to advance our models of galaxy ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/2013/projects13.html -- 21.5 Кб -- 10.04.2016
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    4. SAO Summer Intern Program Projects, 2015
    ... The hot gas in clusters can be perturbed by interactions between clusters. ... investigate the sloshing of the hot gas in the cluster Abell 2204 using deep Chandra ... by mergers with other clusters and by accretion of gas, and the footprints of this ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/2015/projects15.html -- 18.9 Кб -- 10.04.2016
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    5. http://hea-www.harvard.edu/~kim/pap/5ETG_1997.pdf
    ... by the presence of a low surface brightness emission such as that of a cluster gas ... as the result of the dynamical interaction with cluster gas, Forman et al 1979 ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/5ETG_1997.pdf -- 605.2 Кб -- 06.12.2010
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    6. SAO Summer Intern Program Projects, 2004
    ... that reveals the hot intergalactic gas in clusters of galaxies also carries away its ... to cool the gas to low temperatures many times over since the cluster was formed ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects04.html -- 25.0 Кб -- 01.10.2012
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    7. SAO Summer Intern Program Projects, 2014
    ... galaxy clusters to see if this mechanism can explain why some have cold gas, while ... the hot X-ray emitting gas (ICM) that dominates the clusters' baryon distributions ... of the merger, and model the hydrodynamic state of the diffuse cluster gas ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/2014/projects14.html -- 25.2 Кб -- 10.04.2016
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    8. http://hea-www.harvard.edu/~pgreen/SOC/oral3.html
    ... to explain the absence of cold gas in cluster cores, although they appear to be ... and distributions relative to the mass and hot gas of the cluster environment ... the structure of the hot gas in galaxy systems as a function of cluster mass and of ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~pgreen/SOC/oral3.html -- 59.0 Кб -- 01.10.2012
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    9. http://hea-www.harvard.edu/~pgreen/SOC/oral2.html
    ... to explain the absence of cold gas in cluster cores, although they appear to be ... and distributions relative to the mass and hot gas of the cluster environment ... the structure of the hot gas in galaxy systems as a function of cluster mass and of ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~pgreen/SOC/oral2.html -- 61.0 Кб -- 01.10.2012
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    10. http://hea-www.harvard.edu/~pgreen/Papers/um425_05.pdf
    ... Such emission arises from the hot gas bound in massive galaxy clusters or groups. ... indicates that the X-ray ­ emitting gas in the cluster is not See http://asc.harvard ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/um425_05.pdf -- 528.5 Кб -- 14.09.2005
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