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Water masers and the near-stellar environment in YSOs

Published online by Cambridge University Press:  03 August 2017

Mark J. Claussen
Mark J. Claussen*
Affiliation:
National Radio Astronomy Observatory, Array Operations Center, 1003 Lopezville Road, Socorro, NM, 87801 USA

Abstract

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I present a review of observations of water masers, in particular very high angular resolution of water masers using Very Long Baseline Interferometry, with which it is possible to probe the environment of young stellar objects and forming stars within only a few A.U. of the protostar, its accretion disk, and therefore the base of outflowing material. Although reference is made to some high-luminosity sources, the main thrust of the review are the water masers found toward forming objects whose mass and luminosity will be approximately that of the Sun when they reach the main sequence.

Type
Part 1. Star Formation
Information
Symposium - International Astronomical Union , Volume 206: Cosmic Masers: From Protostars to Blackholes , 2002 , pp. 27 - 34
Copyright
Copyright © Astronomical Society of the Pacific 2002 

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