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    71. MEGA
    ... June 2012: Laura Magrini, "Scaling relations of metallicity, stellar mass, and star formation rate in metal-poor starbursts: II ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/colloquia/mega -- 33.9 Кб -- 09.04.2016
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    72. IRAS 20126+4104 (Abstract)
    ... Unveiling the disk-jet system in the massive (proto)star IRAS20126+4104 . Abstract:. ... a single star, then this cannot be a ZAMS star, but more likely a massive protostar which derives its luminosity from accretion ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/i20126_2/abstract.html -- 3.4 Кб -- 11.09.2007
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    73. HAEBEs (Abstract)
    ... The observations reveal the population of young stars that accompanies the formation of intermediate-mass stars. ... star, confirming that the mode of formation of intermediate-mass stars represents the transition between the high-mass and the ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/herbig/abstract.html -- 2.4 Кб -- 11.09.2007
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    74. http://www.arcetri.astro.it/~lt/preprints/hbe_disks/hbe_disks.ps.gz
    ... The existence of accretion disks around massive stars (M> 5 M ) remains a matter of ... constraints to the possi- bility of forming planetary systems around massive stars ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/hbe_disks/hbe_disks.ps.gz -- 152.9 Кб -- 11.09.2007
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    75. http://www.arcetri.astro.it/~fmassi/papers/6438pap.ps.gz
    ... The Vela Molecular Ridge is one of the nearest intermediate­mass star forming regions, located within the galactic plane and ... This is particularly true for massive star forming regions, since they usually are farther away than low­mass star forming ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~fmassi/papers/6438pap.ps.gz -- 262.8 Кб -- 27.02.2007
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    76. http://www.arcetri.astro.it/science/starform/preprints/sepulcre_03.pdf
    ... EDITOR SiO outflows in high-mass star forming regions: A potential chemical clock ... propose that O-B stars form via accretion, in a similar fashion to low-mass stars ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/science/starform/preprints/sepulcre_03.pdf -- 938.6 Кб -- 24.11.2010
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    77. http://www.arcetri.astro.it/~lt/preprints/herbig/herbig.ps.gz
    ... tion of young stars that accompanies the formation of intermediate­mass stars ... mode of formation of intermediate­mass stars represents the transition between the ... At the other extreme, high mass stars are associated with rich clusters with ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/herbig/herbig.ps.gz -- 262.6 Кб -- 11.09.2007
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    78. http://www.arcetri.astro.it/~lt/preprints/bd_disk_cha/ms.ps.gz
    ... to keep the ratio of the disk­to­star mass constant and to the appropriate stellar ... Do they form, as low­mass stars do, from the collapse of a molecular core? ... to the much better known pre­main--sequence low­mass stars, the T Tauri stars (TTS ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/bd_disk_cha/ms.ps.gz -- 82.3 Кб -- 11.09.2007
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    79. Workshops & courses
    ... IAU Symposium 227. May 16-20, 2005 . Massive star birth: a crossroads of astrophysics . European Large Telescope Science Case. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/workshops -- 26.5 Кб -- 09.04.2016
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    80. http://www.arcetri.astro.it/~lt/preprints/proplyds/proplyds.ps.gz
    ... 1997) find that the ages of low mass stars in the Orion Nebula Cluster (ONC) range ... Since the birth a high mass star is expected to halt star formation in its vicinity ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/proplyds/proplyds.ps.gz -- 230.3 Кб -- 11.09.2007
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