Massive molecular outflows

Preprint

16 October 2001

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0110372

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.

Keywords

ESTABLISHED CORRELATIONS
MOLECULAR OUTFLOWS
MASSIVE MOLECULAR
MASSES AND CORE
OUTFLOW MASSES
ORDER A LINEAR
ACCRETION RATE
OUTFLOWS WELL

All Related Versions

Version 1, 2001-10-16, ArXiv
Version 1, 2001-12-21, ArXiv (Unconfirmed version)
Published version: Astronomy & Astrophysics, 383 (3), 892.

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