On the formation of the most massive stars in the galaxy
Roberto J. Galván-Madrid ([Springer, ], 2012)
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| This thesis presents results of Submillimeter Array (SMA) and Very Large Array (VLA) studies of massive star formation regions in the early stages of ionization, as well as an analysis of numerical simulations of the evolution of these young HII regions. The results favor a picture in which very massive stars form in accretion flows that are partially ionized and that keep accreting material from their environment. |
 On the Formation of the Most Massive Stars in the Galaxy.pdf :: Unduh
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| No. Panggil : | e20424989 |
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| Penerbitan : | New York: [Springer, ], 2012 |
| Sumber Pengatalogan: | LibUI eng rda |
| Tipe Konten: | text |
| Tipe Media: | computer |
| Tipe Pembawa: | online resource |
| Deskripsi Fisik: | |
| Tautan: | http://link.springer.com/book/10.1007%2F978-1-4614-3308-8 |
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| No. Panggil | No. Barkod | Ketersediaan |
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| e20424989 | TERSEDIA |
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