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    1. The MACHO Project LMC Variable Star Inventory. X. The R Coronae Borealis Stars
    ... discovery of these new stars increases the number of known RCB stars in the LMC to ... These stars decline much more slowly and are cooler than the RCB stars. ... stars are unknown since there is no direct measurement of the distance to any ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2001ApJ...554..298A.html -- 4.7 Кб -- 21.01.2016
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    2. Dust Around Stars
    ... stars are generally cool stars: M-type giants and supergiants for example, or carbon ... star" spectrum is a carbon-star template spectrum formed from optical, near-infrared ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~volk/dust.html -- 6.7 Кб -- 27.05.2014
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    3. Young, Ultraviolet-bright Stars Dominate Dust Heating in Star-forming Galaxies
    ... Young, Ultraviolet-bright Stars Dominate Dust Heating in Star-forming Galaxies . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2011ApJ...738..124L.html -- 4.2 Кб -- 21.01.2016
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    4. The Mass-loss Return from Evolved Stars to the Large Magellanic Cloud. II. Dust
    ... stars in the Large Magellanic Cloud (LMC) using radiative transfer (RT) models of ... star from each of the bright and faint O-rich AGB populations found by earlier ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2010ApJ...716..878S.html -- 6.0 Кб -- 21.01.2016
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    5. Star formation rates from young-star counts and the structure of the ISM across
    ... Star formation rates from young-star counts and the structure of the ISM across the NGC 346/N66 complex in the SMC . ... stars) locked in young stars is systematically high (књ10 per cent) within the central 15 pc and systematically lower outside ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2015MNRAS.448.1847H.html -- 5.2 Кб -- 21.01.2016
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    6. Stars as Observed in the Infrared
    ... stars hotter than about 3000 K effective temperature radiate like a hot blackbody at ... hotter stars are very close to the same in shape while the cooler K-type giant star ... This is a "hypergiant" star, a very massive somewhat evolved star. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~volk/stars.html -- 4.1 Кб -- 14.06.2010
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    7. Spitzer SAGE-SMC Infrared Photometry of Massive Stars in the Small Magellanic
    ... stars in the Small Magellanic Cloud (SMC), with accurate spectral types compiled ... stars in the Large Magellanic Cloud (LMC), finding that the brightest infrared ... stars among O and early-B stars in our SMC catalog, respectively, when compared to ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2010AJ....140..416B.html -- 5.1 Кб -- 21.01.2016
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    8. Detection of Near-Infrared CO Absorption Bands in R Coronae Borealis Stars
    ... stars are hydrogen-deficient, carbon-rich, pulsating, post-asymptotic giant branch ... eight RCB stars, the RCB-like star DY Per, and the final-helium-flash star FG Sge ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2005AJ....130..256T.html -- 4.6 Кб -- 21.01.2016
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    9. Star Detection
    ... Numerous artifacts around bright stars make star detection very difficult in the linear restorations. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/lindlerd.dir/section3_3.html -- 3.2 Кб -- 15.04.1994
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    10. Birth of Stars and Protoplanetary Systems
    ... Observations show that most stars are formed in multiple star systems and that many have planets. ... JWST Birth of Stars and Protoplanetary Systems theme goal is to unravel the birth and early evolution of stars, from infall on ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/jwst/science/birth-of-stars-protoplanetary-systems -- 16.0 Кб -- 10.04.2016
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