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.

2 pages, 2 ps-figures, in: Proceedings of The earliest phases of massive star birth

References in corpus (3)

• Competitive accretion in embedded stellar cluster
• Massive star formation in 100,000 years from turbulent and pressurized molecular clouds
• A Single Distance Sample of Molecular Outflows from High-Mass Young Stellar Objects

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