ALMA-resolved salt emission traces the chemical footprint and inner wind morphology of VY Canis Majoris

Decin, L, Richards, AMS, Millar, TJ et al. (6 more authors) (2016) ALMA-resolved salt emission traces the chemical footprint and inner wind morphology of VY Canis Majoris. Astronomy & Astrophysics, 592. A76. ISSN 0004-6361

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: © ESO 2016. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: supergiants; stars: mass-loss; circumstellar matter; stars: individual: VY Canis Majoris; astrochemistry; instrumentation: interferometers
Dates:
  • Published: August 2016
  • Accepted: 31 May 2016
  • Published (online): 29 July 2016
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 08 Nov 2016 12:45
Last Modified: 08 Nov 2016 15:29
Published Version: https://doi.org/10.1051/0004-6361/201527934
Status: Published
Publisher: EDP Sciences
Identification Number: https://doi.org/10.1051/0004-6361/201527934

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