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    51. Posters
    ... Previous studies suggest that the planet-forming disks around very-low-mass stars/brown dwarfs may be flatter than those around more massive stars, in contrast to model predictions of larger scale heights for gas-disks around lower-mass stars. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/volatile/posters -- 14.8 Кб -- 10.04.2016
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    52. IAU Symposium 258: The Ages of Stars
    ... Of the fundamental properties that determine the state of a star (mass, composition and age, primarily), we can directly and accurately measure many stars' masses and then estimate the mass of a single star of the same spectral types. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/iau258 -- 15.1 Кб -- 10.04.2016
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    53. STScI Preprint #1192
    ... of the formation of WR stars through mass transfer in close binary systems in ... a detailed quantitative determination of the massive star population in a starburst ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1193/prep1193.html -- 6.4 Кб -- 23.05.2000
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    54. HST this week: 215
    ... Artist's impression of a neutron star . 7 solar mass) stars. ... revealed a strong deficiency of low-mass stars as compared with "normal" globulars ... the cluster re-distributes low-mass stars to larger radii, and therefore renders ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2009/thisweek215.html -- 13.9 Кб -- 23.09.2009
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    55. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_07_24_95
    ... The orbital radial velocity will be measured to provide the mass ratio of the stars. ... 1.12 Completed WF/PC-2 6133 (The Most Massive Stars in the Magellanic Clouds) The WF/PC-2 was used to make observations of star ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_07_24_95 -- 7.8 Кб -- 24.07.1995
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    56. HST this week: 092
    ... Binary Stars in Cyg OB2: Relics of Massive Star Formation in a Super-Star Cluster . ... in the death throes of an extremely massive star, as it collapses to form either a ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/thisweek092.html -- 12.1 Кб -- 08.06.2007
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    57. Dusty HII Regions and Planetary Nebulae
    ... Compact HII regions usually have associated dust from a molecular cloud in which the massive star is being "born". ... early B-type stars there is often a molecular cloud nearby whose dust is heated by the radiation from the massive star or stars ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~volk/features3.html -- 6.2 Кб -- 27.05.2014
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    58. http://www.stsci.edu/science/starburst/Preprints/Tuscany2004.pdf
    ... Abstract Wolf-Rayet stars are the evolved descendents of massive stars ... can b e used for, e.g., inferring a massive star p opulation when the space-UV is ... Conclusions Determining the massive-star IMF in starburst regions often relies on ...
    [ Текст ]  Ссылки http://www.stsci.edu/science/starburst/Preprints/Tuscany2004.pdf -- 378.9 Кб -- 13.08.2004
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    59. http://www.stsci.edu/~jkalirai/PressNGC2099WDs.pdf
    ... astronomers want to know how a rather massive star (up to seven times the mass of ... Depending on the star's initial mass on the main sequence (where a star spends most ...
    [ Текст ]  Ссылки http://www.stsci.edu/~jkalirai/PressNGC2099WDs.pdf -- 323.1 Кб -- 19.09.2008
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    60. HST this week
    ... Coalescence and Accretion Disk Theories of Massive Star Formation with NICMOS ... the environmental influence on the formation of low-mass stars and brown dwarfs ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/thisweek100.html -- 14.8 Кб -- 08.06.2007
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