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    11. SAO Summer Intern Program Projects, 2002
    ... the luminosities of GC X-ray sources in elliptical vs spiral galaxies have also been suggested (see, e.g., Angelini et al. 2001 ... We use the infrared Tully-Fisher relation to determine distances to spiral galaxies in the cluster. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects02.html -- 33.8 Кб -- 01.10.2012
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    12. SAO Summer Intern Program Projects, 2000
    ... This project involves analysing X-ray observations of the nearby spiral galaxy M33. ... point sources in Centaurus A, a merged elliptical and spiral galaxy with an active nucleus, is not significantly different than ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects00.html -- 35.3 Кб -- 01.10.2012
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    13. http://hea-www.harvard.edu/~kim/pap/2008_LMXB_model.pdf
    ... proportional to their X-ray luminosity, and calculated the XLFs of spiral galaxies ... features, such as the luminosity break in the observed XLFs of spiral galaxies ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2008_LMXB_model.pdf -- 1017.9 Кб -- 06.12.2010
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    14. The AstroStat Slog Blog Archive accessing data, easier than before but?
    ... are magnitudes and their errors; positions and their errors; classes like stars, galaxies, AGNs; types or subclasses like elliptical galaxies, spiral galaxies, type I AGN, type Ia, Ib, Ic, and II SNe, various spectral types, etc; estimated variables like ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2009/accessing-data/index.html -- 30.4 Кб -- 01.03.2014
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    15. Aims of ChASeM33?
    ... The engine of spiral galaxy evolution is star formation, which drives the cycling of matter from ISM to stars and back again. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/vlp_m33_public/home2.html -- 6.2 Кб -- 01.10.2012
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    16. http://hea-www.harvard.edu/~pgreen/Morph/MMTmergers_sj2.aux
    ... Mergers (black squares) appear to be similar to spiral galaxies rather than AGN. {\em LOWER PANEL:} Thumbnails for our $18<i<20$ MMT sample have typical component separations $\sim $5$^{\prime \prime }$, and evidence in several cases for multiple nuclei ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~pgreen/Morph/MMTmergers_sj2.aux -- 2.8 Кб -- 12.10.2010
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    17. http://hea-www.harvard.edu/~pgreen/SOC/2.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/2.html -- 15.3 Кб -- 01.10.2012
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    18. http://hea-www.harvard.edu/AstroStat/Stat310_fMMIV/siemiginowska_21sep2004.pdf
    ... s Im ag es f r o m SOHO (So l ar & Hel i o sp h er i c Ob ser vat o r y) The Galaxy Milky Way Spiral Galaxy - similar to Milky Way Stars and Star Clusters Nebulae Cat's Eye Nebula M80- the densest star cluster in Milky Way Extragalactic Objects Op t i cal ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_fMMIV/siemiginowska_21sep2004.pdf -- 1933.7 Кб -- 25.07.2005
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    19. http://hea-www.harvard.edu/~pgreen/SOC/oral3.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/oral3.html -- 59.0 Кб -- 01.10.2012
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    20. http://hea-www.harvard.edu/~kim/pap/2001_M81_ULX.pdf
    ... INTRODUCTION M81 is a nearby early type spiral galaxy well studied in all bands, from radio (e.g.,Beck, Klein, & Krause 1985 ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2001_M81_ULX.pdf -- 273.5 Кб -- 06.12.2010
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