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    31. http://www.arcetri.astro.it/~lt/preprints/s235/s235.ps.gz
    ... that star formation in the cluster is not coeval but proceeds from the outside towards the core of the molecular cloud ... S235 is connected to an extended molecular cloud at ­20 km s \Gamma1 , while S235 A, S235 B and S235 C are embedded in a ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/s235/s235.ps.gz -- 554.0 Кб -- 11.09.2007
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    32. http://www.arcetri.astro.it/~fmassi/papers/6438pap.ps.gz
    ... It is the nearest giant molecular cloud complex hosting massive (although mostly ... massive isolated core lies towards the centre of the molecular cloud (see Fig ... be more consistent with turbulent molecular cloud fragmentation producing a fractal ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~fmassi/papers/6438pap.ps.gz -- 262.8 Кб -- 27.02.2007
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    33. http://www.arcetri.astro.it/~lt/preprints/g962pp/g962pp.pdf
    ... in a neighboring region outside the molecular cloud and normalized to the same area ... AK = 2.6, corresponding to AV = 23, the obscuration caused by the molecular cloud ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/g962pp/g962pp.pdf -- 815.2 Кб -- 11.09.2007
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    34. Fabrizio Massi's home page
    ... Click here for a picture... Current Interests . Near IR photometry of young star clusters . Star forming regions and molecular clouds . NIR. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~fmassi/ -- 3.2 Кб -- 11.03.2015
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    35. http://www.arcetri.astro.it/~lt/preprints/grad_uchii/ms.ps.gz
    ... Introduction Stellar groups form in the dense cores of molecular clouds. ... and molecular­line studies shows that molecular clouds are centrally condensed ... most massive and dense condensations within molecular clouds, and are thought to be ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/grad_uchii/ms.ps.gz -- 88.5 Кб -- 11.09.2007
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    36. EF's Publications
    ... Applications to faint X-ray spectra in the Taurus Molecular Cloud , A , 468 , 501 . ... of X-ray bright variable sources in the Taurus molecular cloud , A , 468 , 485 ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~francio/papers.html -- 41.3 Кб -- 03.02.2016
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    37. http://www.arcetri.astro.it/~comore/pubbl.lis
    ... Water masers associated with dense molecular clouds and ultracompact HII regions ... H2O masers associated with dense molecular clouds and ultracompact HII regions ... 7th Manchester Astronomical Conference on Molecular Clouds, R. James and T. Millar ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~comore/pubbl.lis -- 28.9 Кб -- 17.12.2008
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    38. Ronbun (Abstract)
    ... 2001). We suggest that the embedded stars might be too young to have affected the surrounding molecular cloud significantly on a large scale. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/ronbun/abstract.html -- 3.0 Кб -- 11.09.2007
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    39. http://www.arcetri.astro.it/~lt/projects/ele_lav.ps.gz
    ... star formation in the Cepheus molecular cloud: the S155/Cepheus B interface'', A&A ... formation theories from the Serpens molecular cloud and protocluster'', A&A, 392 ... of the dense cores in the Perseus molecular cloud complex'', A&A, 431, 253 [A68 ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/projects/ele_lav.ps.gz -- 68.1 Кб -- 11.09.2007
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    40. S235 (Abstract)
    ... of the maser features with respect to the molecular cloud velocity imply the presence of highly collimated, energetic and short ... that star formation in the cluster is not coeval but proceeds from the outside towards the core of the molecular cloud ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/s235/abstract.html -- 4.2 Кб -- 11.09.2007
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