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    21. http://hea-www.harvard.edu/~pgreen/SOC/oral2.html
    ... We find that XBONGS are not a single class of object, but fall into four categories -- red early-type galaxies, blue ellipticals, spiral/irregular galaxies and galaxies with AGN colors. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~pgreen/SOC/oral2.html -- 61.0 Кб -- 01.10.2012
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    22. SAO Summer Intern Program Projects, 2005
    ... 10% of the sample and use this complete survey to study the global properties of the galaxies in the sample, including color versus morpological type, color versus luminosity, the interal extinction in spiral galaxies from color versus inclination ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects05.html -- 27.1 Кб -- 01.10.2012
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    23. http://hea-www.harvard.edu/~kim/pap/2012_N1291_Luo.pdf
    ... nearby early-type galaxies and the bulges of nearby spirals (including the Milky Way ... Chandra exposures of nearby elliptical galaxies and spiral bulges have pushed the ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2012_N1291_Luo.pdf -- 990.9 Кб -- 30.08.2012
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    24. SAO Summer Intern Program Projects, 2004
    ... Yet the nature of these galaxies -- dusty elliptical galaxies, star-forming spirals, or `train-wreck' mergers -- has remained elusive because of the small areas and limited spatial resolution of previous mid-IR surveys. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects04.html -- 25.0 Кб -- 01.10.2012
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    25. The AstroStat Slog Blog Archive [MADS] Mahalanobis distance
    ... AJ, 99, 1108 (1990): Kinematics and composition of H II regions in spiral galaxies. II ? M51, M101 and NGC 2403 (Zaritsky, Elston, and Hill) . ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2009/mads-mahalanobis-distance/index.html -- 27.6 Кб -- 01.03.2014
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    26. http://hea-www.harvard.edu/~kim/pap/2007_M33_II.pdf
    ... INTRODUCTION M33 is a late-type spiral galaxy, Sc II Y III, and the third largest galaxy in the Local Group. ... since morphologically it is of intermediate type between the large early-type spiral galaxies and the numerous dwarf galaxies ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2007_M33_II.pdf -- 1006.0 Кб -- 06.12.2010
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    27. http://hea-www.harvard.edu/~elvis/ref_papers.ps
    ... 25 1984 JHKL Photometry of the Nuclei of Normal Spiral Galaxies (S.P. Willner, M. Ward, A. Longmore, A. Lawrence, G. Fabbiano, and M. Elvis) Publi­ cations of the Astronomical Society of the Pacific, volume 96, 143. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~elvis/ref_papers.ps -- 73.3 Кб -- 13.04.2011
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    28. http://hea-www.harvard.edu/~kim/pap/2006_N3379_N4278_XLF.pdf
    ... a clean sample of LMXBs with no contamination by HMXBs, which are likely to contribute to the X-ray source populations of spiral galaxies (the Milky Way and M31) and young or rejuvenated E and S0 galaxies resulting from recent mergers (e.g., NGC 5128 ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2006_N3379_N4278_XLF.pdf -- 358.3 Кб -- 06.12.2010
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    29. http://hea-www.harvard.edu/~kim/pap/2004_M81.pdf
    ... X-ray emission from the nuclear source of the nearby spiral galaxy M81, using the available data collected with ROSAT, ASCA ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2004_M81.pdf -- 504.9 Кб -- 06.12.2010
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    30. http://hea-www.harvard.edu/~kim/pap/CenA_2000.pdf
    ... The extended emission also could be caused by a dustscattering halo, since we are obser ving the nucleus through the dust lane of the merged spiral galaxy. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/CenA_2000.pdf -- 122.0 Кб -- 06.12.2010
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