arXiv · astro-ph/0110372
Massive molecular outflows
Abstract
Well established correlations of low-mass flows show a continuity in the high-mass regime, and mean accretion rates for L>1000 Lsun are dM/dt~10^(-4) Msun/yr. We also present a tight correlation between outflow masses and core masses, which implies that the accretion rate is to first order a linear function of the core mass. All those results support the idea that similar physical processes drive outflows of all masses.
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H. Beuther, P. Schilke, K. M. Menten, C. M. Walmsley, T. K. Sridharan, F. Wyrowski. 2001-10-16. Massive molecular outflows. https://doi.org/10.1051/0004-6361%3A20011808
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