Candidate Water Vapor Lines to Locate the H₂O Snowline through High-dispersion Spectroscopic Observations. I. The Case of a T Tauri Star

Notsu, S, Nomura, H, Ishimoto, D et al. (4 more authors) (2016) Candidate Water Vapor Lines to Locate the H₂O Snowline through High-dispersion Spectroscopic Observations. I. The Case of a T Tauri Star. The Astrophysical Journal, 827 (2). 113. ISSN 0004-637X

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: © 2016 The American Astronomical Society. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: astrochemistry; infrared: planetary systems; ISM: molecules; protoplanetary disks; stars: formation; submillimeter: planetary systems
Dates:
  • Published: 20 August 2016
  • Accepted: 16 June 2016
  • Published (online): 12 August 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 12:17
Last Modified: 08 Nov 2016 15:29
Published Version: https://doi.org/10.3847/0004-637X/827/2/113
Status: Published
Publisher: IOP Publishing
Identification Number: https://doi.org/10.3847/0004-637X/827/2/113

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