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    • [ В начало ] Пред. | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | След.

    81. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Hen.txt
    ... A planetary nebula forms after an aging, low-mass star swells to become a "red giant" and blows off some of its outer layers of ... The current theoretical models do not predict such fast evolution for low-mass stars like that of the Stingray nebula." ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Hen.txt -- 6.4 Кб -- 30.01.2001
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    82. http://www.arcetri.astro.it/~lt/preprints/g962/g962.ps.gz
    ... HII and hot dust emission around young massive stars in G9:62 + 0:19 Leonardo Testi ... first stages of evolution of a young massive star, the source may be observable at K ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/g962/g962.ps.gz -- 288.2 Кб -- 11.09.2007
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    83. http://www.arcetri.astro.it/~lt/preprints/g29g31/maxia.ps.gz
    ... HCs are believed to host young forming massive stars which have been suggested to be ... The importance of the study of high­mass star forma­ tion derives from the close ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/g29g31/maxia.ps.gz -- 386.4 Кб -- 11.09.2007
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    84. http://www.arcetri.astro.it/~sait07/materiainterstellare.pdf
    ... associata (Premio Tacchini) Stars having initial masses between 7-11 M0 (so-called Super-AGB stars) fill the gap between "intermediate-mass'' stars unable to ignite core C-burning and "massive'' stars able to evolve through all nuclear burning stages ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sait07/materiainterstellare.pdf -- 58.9 Кб -- 14.05.2007
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    85. http://www.arcetri.astro.it/~sperello/IAUSymp255p75.pdf
    ... Big Bang material, should have unusually massive stars (a top­heavy IMF), with ... The very massive PopIII stars would then produce a short phase of unusually hard and ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/IAUSymp255p75.pdf -- 284.0 Кб -- 03.03.2009
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    86. http://www.arcetri.astro.it/~lt/preprints/p45maser/p45maser.ps.gz
    ... trace the earliest evolutionary phases of massive stars, much before the onset of an ... thus the ideal indicators of the youngest massive stars which have not yet swept out ... that the bulk of the emission from the youngest massive stars is expected ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/p45maser/p45maser.ps.gz -- 74.0 Кб -- 11.09.2007
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    87. http://www.arcetri.astro.it/irlab/doc/spie_06/6269-46.pdf
    ... is the search for rocky planets with habitable conditions around low-mass stars ... down to a few Earth masses) around low mass stars by means of accurate (few m/s ... mass, rocky planets around cool low-mass stars which are too red for being observed ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/irlab/doc/spie_06/6269-46.pdf -- 328.2 Кб -- 28.04.2006
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    88. http://www.arcetri.astro.it/~olmi/aah4316.pdf
    ... UC) HII regions are used to trace high-mass star formation, and represent a relatively advanced evolutionary stage of a massive ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~olmi/aah4316.pdf -- 794.3 Кб -- 04.11.2005
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    89. http://www.arcetri.astro.it/science/starform/preprints/cesa_23.pdf
    ... evidence of disk-jet systems is found in high-mass star-forming regions ... context of star formation, high-mass stars are commonly defined as those exceeding 8 ... questioning the possibility that high-mass stars can form through (disk) accretion ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/science/starform/preprints/cesa_23.pdf -- 493.9 Кб -- 16.11.2012
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    90. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Tarantula.txt
    ... STScI-PRC99-12 MULTIPLE GENERATIONS OF STARS IN THE TARANTULA NEBULA In the most active starburst region in the local universe lies a cluster of brilliant, massive stars, known to astronomers as Hodge 301. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Tarantula.txt -- 3.9 Кб -- 30.01.2001
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