Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...137...85f&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 137, no. 1, Aug. 1984, p. 85-91.
Astronomy and Astrophysics
Astrophysics
13
Orion Nebula, Star Formation, Stellar Winds, Density Distribution, Pre-Main Sequence Stars, Stellar Mass, Stellar Models, T Tauri Stars, Taurus Constellation
Scientific paper
Using the self-regulated star formation model proposed by Franco and Cox, (1983) the effects of winds from low-mass stars are analyzed. Two types of winds are considered; hypothetical protostellar winds and the observed T Tauri winds. It is found that the radial momentum input, in both cases, could regulate the evolution of the star-forming regions. The birthrates due to protostellar rotationally driven winds and T Tauri winds are very similar, and are proportional to the square root of the local density in the star-forming region. The predicted rates for Taurus-Auriga, Rho Ophiuchi NGC 2264, and the Trapezium region in Orion are in agreement with observational results.
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