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On the formation of the most massive stars in the galaxy

Roberto J. Galván-Madrid ([Springer, ], 2012)

 Abstrak

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.

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No. Panggil : e20424989
Entri utama-Nama orang :
Subjek :
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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