Candidate Water Vapor Lines to Locate the H2O Snowline through High-dispersion Spectroscopic Observations. III. Submillimeter H2 16O and H2 18O Lines

Notsu, S, Nomura, H, Walsh, C orcid.org/0000-0001-6078-786X et al. (4 more authors) (2018) Candidate Water Vapor Lines to Locate the H2O Snowline through High-dispersion Spectroscopic Observations. III. Submillimeter H2 16O and H2 18O Lines. Astrophysical Journal, 855 (1). 62. p. 62. ISSN 0004-637X

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Copyright, Publisher and Additional Information: © 2018. The American Astronomical Society. All rights reserved. This is an author produced version of a paper published in The Astrophysical Journal. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: astrochemistry; ISM: molecules; protoplanetary disks; stars: formation; submillimeter: planetary systems
Dates:
  • Published: 8 March 2018
  • Accepted: 22 January 2018
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: 27 Mar 2018 13:31
Last Modified: 27 Mar 2018 13:31
Published Version: http://iopscience.iop.org/article/10.3847/1538-435...
Status: Published
Publisher: American Astronomical Society
Identification Number: https://doi.org/10.3847/1538-4357/aaaa72

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