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    41. SAO Summer Intern Program Projects, 2011
    ... and that the motions between cores within a clustered region are a factor of two smaller then the large-scale gas motions [2 ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects11.html -- 20.8 Кб -- 01.10.2012
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    42. SAO Summer Intern Program Projects, 2011
    ... and that the motions between cores within a clustered region are a factor of two smaller then the large-scale gas motions [2 ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/2011/projects11.html -- 21.1 Кб -- 01.10.2012
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    43. http://hea-www.harvard.edu/~kim/pap/BinaryQ_2002.pdf
    ... If the lens were a dark cluster lacking not only galaxies but also gas, the gas fraction would have to be $3 times lower than ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/BinaryQ_2002.pdf -- 1062.9 Кб -- 06.12.2010
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    44. Chandra's View of M86
    ... The total gas mass in the plume (7x10 8 M sun ) and tail (1x10 9 M sun ) is about three times that in the core of M86, which supports the scenario where most of the gas was stripped rapidly and recently. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~srandall/M86/ -- 4.0 Кб -- 01.10.2012
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    45. SAO Summer Intern Program Projects, 2012
    ... COMPLETE survey have shown that dense cores in Perseus tend to have very small motions relative to their immediate surroundings, and that the motions between cores within a clustered region are a factor of two smaller then the large-scale gas motions [2 ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/2012/projects12.html -- 20.9 Кб -- 27.02.2014
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    46. http://hea-www.harvard.edu/~pgreen/Papers/Q2345.ps
    ... If the lens were a dark cluster lacking not only galaxies but also gas, the gas fraction would have to be #3 times lower than ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/Q2345.ps -- 2124.2 Кб -- 14.09.2005
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    47. http://hea-www.harvard.edu/x-ray-clusters/papers/nocf-conf.pdf
    ... The central cusp can be characterized by the power-law index of the gas density profile, = d log g /d log r. For uniformity, the radius at which is measured should be chosen at a fixed fraction of the cluster virial radius. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/x-ray-clusters/papers/nocf-conf.pdf -- 480.1 Кб -- 21.11.2006
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    48. The AstroStat Slog massive data
    ... Someone emailed me for globular cluster data sets I used in a proceeding paper ... to understand the data sets with suspicious numbers of globular cluster populations ... On the other hand, obtaining globular cluster data sets was easy because of ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/tag/massive-data/index.html -- 30.0 Кб -- 01.03.2014
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    49. http://hea-www.harvard.edu/vlp_m33_public/rt08a.pdf
    ... stellar clusters (Hunter et al. 1996) and the 'U'-shaped morphology of the X-ray gas ... C1 and C3 is from gas originating from the stellar wind of clusters A and B which ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/vlp_m33_public/rt08a.pdf -- 1183.9 Кб -- 09.06.2008
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    50. The Chandra Multiwavelength Project (ChaMP)
    ... Galactic Plane Survey: > 30 ksecs . No SNR . Galaxies and galaxy clusters: C . ... eq.7 of Burstein Heiles 1978, ApJ, 225 , 40 and assumes a constant dust-to-gas ratio ... C Galaxies and Galaxy clusters (Alexey Vikhlinin): . ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/CHAMP/SURVEY_STRATEGY/merged_list_criteria.html -- 7.0 Кб -- 02.10.2012
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