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    • [ В начало ] Пред. | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | След.

    81. The Orion Nebula Cluster . as a Paradigm of Star Formation
    ... The nearest massive star formation region and the template for massive star- and cluster formation models is then substantially ... Due to magnetic flaring in lower mass stars and shocked winds from high mass stars, X-ray observations are surprisingly ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/orion/talksList -- 54.3 Кб -- 10.04.2016
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    82. http://www.stsci.edu/ftp/stsci/library/abstracts/1142.abs
    ... Institute\\ \\ 3700 San Martin Drive\\ \\ Baltimore, MD 21218} \pub{{\em the proceedings of}\\ ~\\ Luminous Blue Variables: Massive Stars in Transition\\ ~\\ {\em held October 1996 in Kona, Hawaii}} \maketitle \begin{abstract} Nebula around LBVs have ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/stsci/library/abstracts/1142.abs -- 2.4 Кб -- 25.04.1997
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    83. HST this week: 056
    ... A Paschen-Alpha Study of Massive Stars and the ISM in the Galactic Center . ... dwarfs are the evolutionary end point for most stars with masses less than ~7 M Sun ... to the IMF above ~1 M Sun (high mass stars are rare, so high mass remnants, like ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2008/thisweek056.html -- 16.9 Кб -- 25.02.2008
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    84. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_01_23_96
    ... WF/PC-2 was used to make observations of the low mass binary = stars RHY064 and RHY402 (M-class dwarf stars) which are located ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_01_23_96 -- 6.4 Кб -- 23.01.1996
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    85. http://www.stsci.edu/~jkalirai/PressN6397WhiteDwarfs.pdf
    ... stars burned out as white dwarfs, they were among the most massive stars in NGC 6397 ... Because massive stars are thought to gather at a globular cluster's core ... Globular clusters sort out stars according to their mass, governed by a ...
    [ Текст ]  Ссылки http://www.stsci.edu/~jkalirai/PressN6397WhiteDwarfs.pdf -- 91.8 Кб -- 19.09.2008
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    86. http://www.stsci.edu/ftp/observing/status_reports/old_reports_00/hst_status_07_25_00
    ... Observations were also made of several reference stars. Our goal is to measure the masses of low mass young stars. ... 1.14 Completed WF/PC-2/STIS/CCD 8675 (The Massive Star Content of NGC 6822) The WF/PC-2 and the Space Telescope Imaging ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_00/hst_status_07_25_00 -- 10.5 Кб -- 25.07.2000
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    87. HST this week: 242
    ... NGC 3603 is a massive star-forming region located in Carina spiral arm at a distance ... centering around 1 Myr for the massive stars, alkthough there are some suggestions ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2010/thisweek242.html -- 18.7 Кб -- 31.01.2011
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    88. Astrophysics in the Next Decade
    ... contributions made to ISM dust enrichment by low and intermediate mass stars (AGB, post-AGB and PN phases) and by massive stars ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/jwst2007/talksList -- 27.8 Кб -- 10.04.2016
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    89. http://www.stsci.edu/ftp/observing/status_reports/hst_status_03_26_02
    ... of Some of the Galaxy's Most Massive Stars) Fine Guidance Sensor #1 was used to make ... luminosity function {LF} of star forming regions which produce such high mass stars ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/hst_status_03_26_02 -- 8.4 Кб -- 26.03.2002
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    90. About IAU Symposium 258
    ... Of the fundamental properties that determine the state of a star (mass, composition and age, primarily), we can directly and ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/iau258/rationale -- 22.0 Кб -- 10.04.2016
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