Statistics – Computation
Scientific paper
Jan 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15...24r&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Jan. 1989, p. 24-28. In Russian. In Russian. In Russian.
Statistics
Computation
Protostars, Star Formation, Stellar Evolution, Stellar Models, Computational Astrophysics, Stellar Mass
Scientific paper
The velocity of a self-propagating star formation wave is calculated. A
model which accounts for the nonlocal character of induced star
formation and the finite time of evolution of protostars is used.
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