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    41. Arcetri Star-Formation Group Publications
    ... 2000, A , in press . Abundance profiles of CH3OH and H2CO toward massive young stars as tests of gas-grain chemical models . ... The onset of cluster formation around intermediate-mass stars . L. Testi, F. Palla, A. Natta . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/starform/publ2000.htm -- 12.8 Кб -- 21.06.2001
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    42. Arcetri Star-Formation Group Publications
    ... 2010, A , in press . SiO outflows in high-mass star forming regions: A potential chemical clock? ... Class I and Class II methanol masers in high-mass star forming regions . F. Fontani, R. Cesaroni, R. S. Furuya . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/starform/publ2010.htm -- 7.0 Кб -- 26.03.2012
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    43. http://www.arcetri.astro.it/~lt/projects/ele_lav.ps.gz
    ... M., 1998, ``HII and hot dust emission around young massive stars in G 9.62+0.19'', A ... L., Felli M., Taylor G.B., 1999, ``Young massive stars in the ISOGAL survey I. VLA ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/projects/ele_lav.ps.gz -- 68.1 Кб -- 11.09.2007
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    44. http://www.arcetri.astro.it/~lt/preprints/tegami/tegami.ps.gz
    ... at millimeter wavelengths of the high­ mass star forming region G24.78+0.08, where a ... Introduction High­mass stars are usually defined as stars with mass above ё8 M fi ... Moreover, massive stars form in clusters, which not only complicates the ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/tegami/tegami.ps.gz -- 189.9 Кб -- 11.09.2007
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    45. http://www.arcetri.astro.it/~lt/preprints/tegami/tegami.pdf
    ... at millimeter wavelengths of the high-mass star forming region G24.78+0.08, where a ... Introduction High-mass stars are usually defined as stars with mass above 8 M : for ... Moreover, massive stars form in clusters, which not only complicates the ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/tegami/tegami.pdf -- 221.6 Кб -- 11.09.2007
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    46. G 9.62+0.19 (Abstract)
    ... HII and hot dust emission around young massive stars in G9.62+0.19 . Abstract:. ... that explains why, in the first stages of evolution of a young massive star, the source may be observable at K but not in the ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/g962/abstract.html -- 3.3 Кб -- 11.09.2007
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    47. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Ciclo.txt
    ... A torrent of ionizing radiation and fast stellar winds from these massive stars has blown a large cavity around the cluster. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Ciclo.txt -- 3.6 Кб -- 30.01.2001
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    48. http://www.arcetri.astro.it/~lt/preprints/g962f/g962.ps.gz
    ... This is the first direct evidence that a newly born massive star is powering the G9.62+0.19­F hot core. ... Introduction The formation of massive stars (M– 10 M fi ) has received growing attention in recent years, because of their ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/g962f/g962.ps.gz -- 319.5 Кб -- 11.09.2007
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    49. Arcetri Star-Formation Group Publications
    ... 2001, A , in press . On the formation of primordial massive stars . K. Omukai, Francesco Palla . 2001, ApJL, in press . ... 2001, A , in press . Disks around intermediate-mass stars and protostars . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/starform/publ2001.htm -- 17.2 Кб -- 07.03.2002
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    50. http://www.arcetri.astro.it/~palla/webpage/Biblio.pdf
    ... 1990, Astrophys. J. Lett., 360, L47. The Birthline for Intermediate Mass Stars 20. ... Infrared studies of pre-main-sequence intermediate mass stars: LkH 198 27. ... J., 414, 418 The Pre-Main-Sequence evolution of intermediate-mass stars 30. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~palla/webpage/Biblio.pdf -- 127.6 Кб -- 21.09.2007
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