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    1. Cold dust in three massive evolved stars in the LMC
    ... Cold dust in three massive evolved stars in the LMC . Boyer, M. L., Sargent, B., van Loon, J. Th., ... 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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    2. May Symposium 2006
    ... 2006 May Symposium . Massive Stars: From Pop III and GRBs to the Milky Way. ... The title was: Massive Stars: From Pop III and GRBs to the Milky Way . ... in the general areas of: the formation of massive stars (both Pop III and in the ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/may_symp -- 17.9 Кб -- 10.04.2016
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    3. http://www.stsci.edu/institute/conference/iausps13/presentations/Przybilla.pdf
    ... CNO in Massive Stars Norbert Przybilla & Maria-Fernanda Nieva Dr. Remeis-Observatory Bamberg CNO in Massive Stars IAU XXVIII GA SpS13 ­ 28.08.2012 Intro Question What information can massive stars in the solar neighbourhood provide on the solar CNO ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/iausps13/presentations/Przybilla.pdf -- 1472.4 Кб -- 05.02.2013
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    4. The Infrared Properties of Massive Stars in the Magellanic Clouds
    ... The Infrared Properties of Massive Stars in the Magellanic Clouds . ... highlights of our study of the infrared properties of massive stars in the Large and Small Magellanic Clouds (from Bonanos et ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2011BSRSL..80..346B.html -- 4.0 Кб -- 22.08.2014
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    5. Spitzer View of Young Massive Stars in the Large Magellanic Cloud H II Complex
    ... Spitzer View of Young Massive Stars in the Large Magellanic Cloud H II Complex N 44 . ... conditions to illustrate a correlation between the current formation of O-type stars and previous formation of massive stars ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2009ApJ...695..511C.html -- 4.7 Кб -- 21.01.2016
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    6. Spitzer SAGE-SMC Infrared Photometry of Massive Stars in the Small Magellanic
    ... Spitzer SAGE-SMC Infrared Photometry of Massive Stars in the Small Magellanic Cloud . ... We present a catalog of 5324 massive stars in the Small Magellanic Cloud (SMC), with accurate spectral types compiled from the ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2010AJ....140..416B.html -- 5.1 Кб -- 21.01.2016
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    7. http://www.stsci.edu/institute/conference/may_symp/supportingFiles/talk28
    ... AN X-RAY TOUR OF MASSIVE STAR-FORMING REGIONS WITH CHANDRA Not Your Grandmother's ... to SNR) in the life cycle of massive stars and their effects on their surroundings ... Massive stars often show surprisingly hard X-ray emission ­ this may be a new ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/may_symp/supportingFiles/talk28 -- 2084.9 Кб -- 11.05.2006
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    8. HST Observer Monthly
    ... University of Sheffield Title = "A Massive Star Census of the Starburst Cluster R136 ... 2010, most astronomers believed the most massive stars in the universe were roughly ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/observermonthly/2012/apr1 -- 15.7 Кб -- 10.04.2016
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    9. May Symposium
    ... Chair: Jennifer Wiseman . 9:10 - 9:40am . Theories of Massive Star Formation . Mark Krumholz . 9:40 - 9:55am . Discussion . ... BREAK . 11:10 - 11:40am . Observations of Massive Star Formation . Nimesh Patel . 11:40 - 11:55am . Discussion . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/may_symp/agenda -- 23.7 Кб -- 10.04.2016
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    10. Rodolfo Barba
    ... Way which would provide empirical estimates of their masses. b) Massive stars groups: the knowledge of the stellar content of ... 30 Doradus, in the LMC, putting emphasis on the new stellar generation, where massive proto-star candidates are placed ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/jamb98/node3.html -- 3.8 Кб -- 24.03.1998
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