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    1. SAO Summer Intern Program
    ... in which one of the stars is a red dwarf and the other star is a compact object, a ... in which one of the stars is a red dwarf losing mass to the other star which is a ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects98.html -- 16.5 Кб -- 01.10.2012
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    2. SAO Summer Intern Program Projects, 2002
    ... are interacting binary stars; the two stars are a white dwarf and a red dwarf ... The red dwarf donates mass via a mass transfer stream. ... strength dictates the dynamics from the moment the material leaves the red dwarf ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects02.html -- 33.8 Кб -- 01.10.2012
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    3. http://hea-www.harvard.edu/~pgreen/Papers/irdas00.pdf
    ... a near-IR photometric search for cool red dwarf companions to hot white dwarfs (WDs ... nor the mass estimate of the red dwarf companion correlate with white dwarf mass, as ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/irdas00.pdf -- 224.6 Кб -- 12.02.2002
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    4. http://hea-www.harvard.edu/~pgreen/Papers/irdas00.ps
    ... a near­IR photometric search for cool red dwarf companions to hot white dwarfs (WDs ... nor the mass estimate of the red dwarf companion correlate with white dwarf mass, as ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/irdas00.ps -- 677.6 Кб -- 12.02.2002
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    5. SAO Summer Intern Program Projects, 1999
    ... binary stars in which one star is a red dwarf that is losing mass to the other star ... red interloper has been detected in the vicinity of the faint Tremendous Outburst ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects99.html -- 36.2 Кб -- 01.10.2012
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    6. http://hea-www.harvard.edu/~pgreen/Papers/Green13.pdf
    ... 1991). Red dwarfs and red subdwarfs are low-mass main-sequence stars. ... Other dC stars (black dots) appear to fall between the red dwarfs (densest region on the right) and the subdwarfs (lower ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/Green13.pdf -- 2709.7 Кб -- 12.02.2013
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    7. http://hea-www.harvard.edu/~pgreen/Papers/euvdas99.pdf
    ... A number of interacting binary systems where the WD is the primary (i.e., optically brightest) star have also been found among EUV-detected systems (e.g., six close, interacting WD/red dwarf binaries by Vennes & Thorstensen 1994). ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/euvdas99.pdf -- 712.5 Кб -- 19.09.2005
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    8. http://hea-www.harvard.edu/~pgreen/figs/cdwarfs2.ps
    ... The Dark Matter Main sequence stars, red giants, white dwarfs ­ these are three among the many types of stars that populate a galaxy. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/figs/cdwarfs2.ps -- 62.1 Кб -- 22.11.1995
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    9. http://hea-www.harvard.edu/~pgreen/Papers/euvdas99.ps
    ... A number of interacting binary systems where the WD is the primary (i.e., optically brightest) star have also been found among EUV­detected systems (e.g., six close, inter­ acting WD/red dwarf binaries by Vennes & Thorstensen 1994). ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/euvdas99.ps -- 2683.7 Кб -- 19.09.2005
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    10. SAO Summer Intern Program Projects, 2004
    ... Symbiotic stars are binary star systems in which a red-giant star and a white-dwarf star orbit one another. ... The companion white dwarf has a very strong surface gravitational field, and it captures a portion of the red-giant wind as it ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects04.html -- 25.0 Кб -- 01.10.2012
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