Infall and outflow within 400 AU from a high-mass protostar. 3-D velocity fields from methanol and water masers in AFLG 5142

Details Infall and outflow within 400 AU from a high-mass protostar. 3-D velocity fields from methanol and water masers in AFLG 5142 Infall and outflow within 400 AU from a high-mass protostar. 3-D velocity fields from methanol and water masers in AFLG 5142

2011-10-07

arxiv.org/abs/1110.1647v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

6 pages, 4 figures, 1 table, accepted for publication in A&A Letters

Scientific paper

Observational signatures of infalling envelopes and outflowing material in early stages of protostellar evolution, and at small radii from the protostar, are essential to progress in the understanding of the mass-accretion process in star formation. In this letter, we report a detailed study of the accretion and outflow structure around a protostar in the well-known high-mass star-forming region AFGL 5142. We focus on the mm source MM-1, which exhibits hot-core chemistry, radio continuum emission, and strong water and methanol masers. Remarkably, our Very Long Baseline Interferometry (VLBI) observations of molecular masers over six years provided us with the 3-D velocity field of circumstellar molecular gas with a resolution of 0.001-0.005 arcseconds and at radii <0.23 arcseconds (or 400 AU) from the protostar. In particular, our measurements of methanol maser emission enabled, for the first time, a direct measurement of infall of a molecular envelope (radius of 300 AU and velocity of 5 km/s) onto an intermediate- to high-mass protostar. We estimate an infall rate of 0.0006 n_8 Msun/year, where n_8 is the ambient volume density in units of 10^8 cm-3 (required for maser excitation). In addition, our measurements of water maser (and radio continuum) emission identify a collimated bipolar molecular outflow (and ionized jet) from MM-1. The evidence of simultaneous accretion and outflow at small spatial scales, makes AFGL 5142 an extremely compelling target for high-angular resolution studies of high-mass star formation.

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