Ionized Gas Towards Molecular Clumps: Physical Properties of Massive Star Forming Regions

Johnston, KG, Shepherd, DS, Aguirre, JE et al. (3 more authors) (2009) Ionized Gas Towards Molecular Clumps: Physical Properties of Massive Star Forming Regions. The Astrophysical Journal, 707 (1). pp. 283-309. ISSN 0004-637X

Abstract

Metadata

Authors/Creators:
  • Johnston, KG
  • Shepherd, DS
  • Aguirre, JE
  • Dunham, MK
  • Rosolowsky, E
  • Wood, K
Copyright, Publisher and Additional Information: (c) 2009, The American Astronomical Society. All rights reserved. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: circumstellar matter; H ii regions; radio continuum: stars; stars: formation; stars: winds, outflows
Dates:
  • Published: 10 December 2009
  • Accepted: 29 September 2009
  • Published (online): 20 November 2009
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 14 Feb 2017 14:14
Last Modified: 14 Feb 2017 14:14
Published Version: https://doi.org/10.1088/0004-637X/707/1/283
Status: Published
Publisher: American Astronomical Society
Identification Number: https://doi.org/10.1088/0004-637X/707/1/283

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Filename: Johnston_2009_ApJ_707_283.pdf

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