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    91. http://hea-www.harvard.edu/CHAMP/PUBLICATIONS/jds_santander.ps
    ... The remaining counterparts are either stars (8%) or galaxy clusters (1%). ... 1 ), normal galaxies with absorption lines (12%), stars (8%) and galaxy clusters (1 ... that is so heavily enshrouded by dust and gas that only hard X­rays can escape the ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/CHAMP/PUBLICATIONS/jds_santander.ps -- 741.4 Кб -- 19.09.2003
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    92. http://hea-www.harvard.edu/~pgreen/Papers/hs1216_04.ps
    ... cluster­scale masses that failed to make substantial galaxies (i.e. `dark clusters ... cluster, the minimum flux redshift is about 0.7, for which the expected X­ray flux ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/hs1216_04.ps -- 773.4 Кб -- 14.09.2005
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    93. AstroStat Talks 2014-2015
    ... seeded region growing (G-SRG) method for clustering and detecting source structures ... that X-ray binary systems appear to cluster based on their compact object type when ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1415/ -- 48.3 Кб -- 10.04.2016
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    94. http://hea-www.harvard.edu/~rsmith/cv/Bibliography.pdf
    ... 143 "Probing the Outskirts of the Early Stage Galaxy Cluster Merger A1750", Bulbul, Esra, Randall, Scott W., Bayliss, Matthew ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~rsmith/cv/Bibliography.pdf -- 110.3 Кб -- 23.03.2016
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    95. http://hea-www.harvard.edu/~pgreen/Papers/lbqsspec96.ps
    ... Assuming that RL QSOs are probably giant ellipticals in clusters, those authors postulate that the absorption 22 N. Schartel et al. is associated with cold intracluster gas (e.g., cooling flows). ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/lbqsspec96.ps -- 259.3 Кб -- 30.07.1996
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    96. http://hea-www.harvard.edu/~kim/pap/2005_ChaMP_hard_AGN.pdf
    ... galaxies (24%), absorption line galaxies (7%), stars (5%), or clusters (2 ... quasars and lower luminosity Seyfert galaxies with significant absorbing gas columns ... The study of AGNs enshrouded by dust and gas is not new. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2005_ChaMP_hard_AGN.pdf -- 1020.4 Кб -- 06.12.2010
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    97. SAO Summer Intern Program Projects, 2009
    ... The intern working with me will learn about stars and star clusters, and how to use high-resolution spectra of stars to determine their properties, whether they are members of a cluster or not, and if they have any close unseen companions. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects09.html -- 25.2 Кб -- 01.10.2012
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    98. SAO Summer Intern Program Projects, 2009
    ... The intern working with me will learn about stars and star clusters, and how to use high-resolution spectra of stars to determine their properties, whether they are members of a cluster or not, and if they have any close unseen companions. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/2009/projects09.html -- 25.5 Кб -- 01.10.2012
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    99. bkgd
    ... telescope Chandra observes ( in order of size ) Galactic Clusters , galaxies , Quasars , Supernovae , Pulsars , nebula , X-ray ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/CHAMP/EDUCATION/PUBLIC/bkgd.html -- 11.4 Кб -- 02.10.2012
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    100. http://hea-www.harvard.edu/~elvis/extreme_SPIE06.pdf
    ... clusters of galaxies; · thermonuclear burning in X-ray bursts; · element abundances ... Gas Polarimeter has the moderate energy resolution typical URL: http://www-conf.slac ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~elvis/extreme_SPIE06.pdf -- 128.1 Кб -- 13.04.2011
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