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    51. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ViaLattea/9926.txt
    ... bright red giants, which are stars similar to the Sun in mass that are nearing the ... to be unusually young and more massive than the other stars in a globular cluster ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ViaLattea/9926.txt -- 5.1 Кб -- 02.03.2001
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    52. Arcetri Star-Formation Group Publications
    ... Anatomy of a high-mass star forming cloud: the G24.78+0.08 (proto)stellar cluster . R. Cesaroni, C. Codella, R.S. Furuya, L. Testi . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/starform/publ2003.htm -- 12.9 Кб -- 18.12.2003
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    53. The puzzling core of the Phoenix cluster: deep X-ray observations
    ... cooling gas would be to feed massive star formation episodes in the central galaxy ... However, the observed lack of massive star formation events and of large reservoirs ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/previous/204-scientific-news/916-phoenix-tozzi -- 28.5 Кб -- 10.04.2016
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    54. http://www.arcetri.astro.it/~fmassi/projects/eng.curr.pdf
    ... Triggered Massive-Star Formation on the Borders of Galactic HII Regions II. ... Triggered Massive-Star Formation on the Borders of Galactic HI I Regions. ... Triggered Massive-Star Formation on the Borders of Galactic HII Regions" in Cesaroni ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~fmassi/projects/eng.curr.pdf -- 112.1 Кб -- 02.12.2015
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    55. http://www.arcetri.astro.it/~palla/webpage/fp_pubbl.pdf
    ... The Birthline for Intermediate Mass Stars [A20] Palla, F.: 1991, Invited Review at ... studies of pre­main-sequence intermediate mass stars: LkH 198 [A27] Natta, A., Palla ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~palla/webpage/fp_pubbl.pdf -- 99.9 Кб -- 02.03.2014
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    56. http://www.arcetri.astro.it/~lt/preprints/haebe3/7985.ps.gz
    ... low density aggregates of T Tauri stars and the dense clusters around massive stars ... Only the most massive stars (10­20 M fi ) are found to be associated with dense ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/haebe3/7985.ps.gz -- 174.0 Кб -- 11.09.2007
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    57. http://www.arcetri.astro.it/science/starform/preprints/cesa_27.pdf
    ... This result suggests that high-mass stars and/or stellar clusters containing young massive stars may continue to accrete for a ... However, massive stars form in clusters (e.g., Tan et al. 2014), and it is likely that multiple stars contribute to the ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/science/starform/preprints/cesa_27.pdf -- 121.2 Кб -- 19.02.2016
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    58. http://www.arcetri.astro.it/science/starform/preprints/codella_17.pdf
    ... c ESO 2011 On the kinematics of massive star forming regions: the case of IRAS 17233 ... would help to discriminate between different models of formation of massive stars ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/science/starform/preprints/codella_17.pdf -- 1177.9 Кб -- 30.03.2011
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    59. http://www.arcetri.astro.it/radtran/talks/cvlahakis.pdf
    ... both FIR and radio emission caused by high-mass stars FIR emission dust heating massive stars supernovae relativistic electrons ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/radtran/talks/cvlahakis.pdf -- 460.3 Кб -- 25.06.2007
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    60. http://www.arcetri.astro.it/~sait07/posters.pdf
    ... compatible with that obtained by Skumanich (1972) for 1 solar mass stars, and extends its applicability to a broader range of ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sait07/posters.pdf -- 84.3 Кб -- 15.05.2007
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