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    41. http://www.arcetri.astro.it/~sbianchi/clumping/paper.ps
    ... from the observed properties of Giant Molecular Clouds and molecular gas in the ... atomic gas and clumps associated to high density Gi­ ant Molecular Clouds (GMCs ... pc: a cubic cell of 36 pc will therefore have the same volume as a molecular cloud ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sbianchi/clumping/paper.ps -- 633.7 Кб -- 24.08.1999
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    42. http://www.arcetri.astro.it/~lt/preprints/i20126_deb/pp2.ps.gz
    ... between the energetic outflowing material and the surrounding molecular cloud ... 300 M fi molecular cloud and the mass of the disk plus circumstellar envelope traced ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/i20126_deb/pp2.ps.gz -- 65.9 Кб -- 11.09.2007
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    43. http://www.arcetri.astro.it/~lt/preprints/w75n_sio/w75n_sio.ps.gz
    ... is expected in the ambient component of molecular clouds with active star formation ... of 10 6 over that found in quiescent molecular clouds and can delineate the axis of ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/w75n_sio/w75n_sio.ps.gz -- 503.4 Кб -- 11.09.2007
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    44. http://www.arcetri.astro.it/~fmassi/papers/3836pap.ps.gz
    ... star clusters in the Vela­D molecular cloud, all associated with luminous (# 10 3 L ... 7 % of embedded clusters emerge from molecular clouds to become bound clusters of ... in complete samples of lu­ minous embedded sources in giant molecular clouds ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~fmassi/papers/3836pap.ps.gz -- 528.7 Кб -- 29.11.2005
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    45. Francesco Fontani's Curriculum Vitae
    ... Molecular clouds and formation of high-mass stars: multi-line observations of the molecule CH 3 CCH.) ... pc-scale molecular clouds hosting massive star formation . Maser emission . Molecular outflows and jets . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~fontani/curriculum.html -- 3.6 Кб -- 01.10.2012
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    46. IRAS 20126+4104 - OVRO (Abstract)
    ... 300 Msun molecular cloud and the mass of the disk plus circumstellar envelope traced by millimeter continuum emission is ~50 Msun. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/i20126_deb/abstract.html -- 3.3 Кб -- 11.09.2007
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    47. http://www.arcetri.astro.it/~fmassi/papers/ms1.pdf
    ... complex is composed of at least three molecular clouds, named A, C and D (Murphy ... those obtained for the Orion molecular cloud which possesses similar characteristics ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~fmassi/papers/ms1.pdf -- 2003.5 Кб -- 03.10.2006
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    48. G35.20-1.74 (Abstract)
    ... IR cluster (where most probably it has already come to an end) but is still taking place in other parts of the molecular cloud ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/g3520/abstract.html -- 3.6 Кб -- 11.09.2007
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    49. LEONARDO TESTI - SCIENTIFIC PUBLICATIONS
    ... 48) - Constraints on star formation theories from the Serpens molecular cloud and protocluster . L. Olmi & L. Testi . ... 4) - Stimulated Star Formation in the Cepheus Molecular Cloud: The S155/Cepheus B interface . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/preprints.html -- 107.6 Кб -- 11.09.2007
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    50. Astrobigne 2014-2015
    ... main reservoir HD is initiated in molecular clouds by exothermic gas-phase reactions ... long been used as tracers of the coldens and densest portions of molecular clouds ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/home-italiano/202-seminari/930-astrobigne-2014-2015 -- 68.0 Кб -- 10.04.2016
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