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    1. GSAOI Orion Nebula Cluster Science Page
    ... Gemini South Adaptive Optics Imager (GSAOI) . The Orion Nebula - A Detailed Study of a Nearby Massive Star-Forming Region:. ... mass function, i.e., the number of stars of each mass that have formed, in this region of intense massive star formation ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gsaoi/science/orion.shtml -- 6.7 Кб -- 01.10.2012
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    2. GSAOI Super Star Clusters Science Page
    ... Understanding the stellar populations in these massive star-forming regions, and in particular the interplay between high- and ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gsaoi/science/ssc.shtml -- 6.0 Кб -- 01.10.2012
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    3. http://www.mso.anu.edu.au/seminars/abstracts/20150205-1100.html
    ... The low-mass stars, with ages comparable to the age of the Universe, retain the ... Low- to intermediate-mass stars end their nuclear burning life on the AGB. ... of stellar models of low- and intermediate-mass AGB stars at Z = 0.001 ([Fe/H] = -1 ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150205-1100.html -- 6.1 Кб -- 10.04.2016
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    4. http://www.mso.anu.edu.au/seminars/abstracts/20150402-1100.html
    ... Jeremy Goodman . "Very Massive Stars". ... I will show that quasar disks may form stars with masses much larger than in giant molecular clouds. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150402-1100.html -- 4.4 Кб -- 10.04.2016
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    5. COALA - Computational Astrophysics Laboratory
    ... Low and intermediate-mass red giant stars played an important role in this story, by producing much of the carbon, nitrogen ... Asymptotic Giant Blanch (AGB) Stars: For low and intermediate-mass stars (with initial masses between about 0.8 to 8 solar ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/coala/star.html -- 6.0 Кб -- 01.10.2012
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    6. http://www.mso.anu.edu.au/seminars/abstracts/20150528-1100.html
    ... George Zhou . "Discovering and characterising transiting planets and low mass stars". ... will present discoveries of new transiting planets and low mass stars, and the characterisation of their fundamental properties ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150528-1100.html -- 4.9 Кб -- 10.04.2016
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    7. http://www.mso.anu.edu.au/seminars/abstracts/20150409-1100.html
    ... Between 30% and 80% of the mass of the star is lost in an extreme stellar wind. ... The mass loss of Sun-like stars is crucial to both stellar and galactic evolution ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150409-1100.html -- 4.9 Кб -- 10.04.2016
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    8. GSAOI Magellanic Cloud Planetary Nebulae Science Page
    ... Theoretical evolutionary tracks predict that all stars with masses in the range 1.4 ... According to the models, much of the mass of these stars is lost during a series of ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gsaoi/science/pne.shtml -- 8.4 Кб -- 01.10.2012
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    9. The High-Z SN Search Description
    ... After Helium, these massive stars convert their Carbon to Oxygen, and then into ... One good guess is the the Eta Carinae, one of the most massive stars in our galaxy. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~brian/PUBLIC/supernovae.html -- 12.8 Кб -- 01.10.2012
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    10. http://www.mso.anu.edu.au/~charley/papers/RoblesLineweaver2006.pdf
    ... the mass and non­binarity of the Sun in anthropic terms: more massive stars would not allow the time needed for life to evolve ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/RoblesLineweaver2006.pdf -- 68.9 Кб -- 01.05.2007
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