Massive molecular outflows

Astronomy and Astrophysics – Astrophysics

Scientific paper

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

Scientific paper

10.1051/0004-6361:20011808

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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