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    21. Cold dust in three massive evolved stars in the LMC
    ... We model the spectral energy distributions using radiative transfer codes and find that these three stars have mass-loss rates up to 10-3 M_тКЩ yr-1, suggesting that high-mass stars are important contributors to the life-cycle of dust. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2010A&A...518L.142B.html -- 4.4 Кб -- 21.01.2016
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    22. Herschel Exploitation of Local Galaxy Andromeda (HELGA). III. The Star
    ... Herschel Exploitation of Local Galaxy Andromeda (HELGA). III. The Star Formation Law in M31 . ... We present a detailed study of how the star formation rate (SFR) relates to the interstellar medium (ISM) of M31 at ~140 pc ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2013ApJ...769...55F.html -- 5.0 Кб -- 21.01.2016
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    23. The Mass Loss Return from Evolved Stars to the Large Magellanic Cloud:
    ... The Mass Loss Return from Evolved Stars to the Large Magellanic Cloud: Empirical Relations for Excess Emission at 8 and 24 ЮМm ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2009AJ....137.4810S.html -- 5.6 Кб -- 21.01.2016
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    24. http://www.stsci.edu/instrument-news/handbooks/nicmos/c14_calplan.doc6.html
    ... stars in the appropriate flux range for NICMOS, M. Rieke, R. Thompson, and ... star lists used by ground-based telescopes are inadequate for NICMOS because they ... The star selection is based upon HST Guide Star Availability/Suitability Windows. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/nicmos/c14_calplan.doc6.html -- 10.7 Кб -- 07.08.1997
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    25. A Population of Accreted Small Magellanic Cloud Stars in the Large Magellanic
    ... We measure metallicities from the Ca triplet lines of ~1000 LMC field stars and 30 stars in the kinematically distinct population. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2011ApJ...737...29O.html -- 5.0 Кб -- 21.01.2016
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    26. Variable Evolved Stars and Young Stellar Objects Discovered in the Large
    ... 66%) of the extreme AGB stars are variable and only smaller fractions of carbon-rich (6.1%) and oxygen-rich (2.0%) stars are detected as variable sources. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2009AJ....137.3139V.html -- 4.4 Кб -- 21.01.2016
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    27. Spencer's star
    ... Spencer's star is the central star in this picture, which is taken from the Digital ... stars visible on these images are approximately 1 million times fainter than the ... star is almost midway between the region marked M48 and the star Procyon, the ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/dogstar.html -- 2.3 Кб -- 08.06.2007
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    28. Comparisons of Implementations
    ... star cluster, shown in the left panel of Fig. 1 , consists of a field of unresolved ... location (tb, eb/tb) for each star in the star cluster for restorations based on the ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/snyderd.dir/section3_3.html -- 10.8 Кб -- 18.04.1994
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    29. The Orion Nebula Cluster . as a Paradigm of Star Formation
    ... As the nearest young cluster dominated by massive OB stars, the Orion Nebula Cluster plays a paradigmatic role in our understanding of star and planet formation. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/orion -- 14.8 Кб -- 10.04.2016
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    30. Spatially Resolved Ultraviolet, HЮБ, Infrared, and Radio Star Formation in M81
    ... Spatially Resolved Ultraviolet, HЮБ, Infrared, and Radio Star Formation in M81 . ... design nature of M81 is clearly seen, showing two well-resolved spiral arms containing numerous bright star-forming regions ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2004ApJS..154..215G.html -- 4.6 Кб -- 21.01.2016
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