Characterising the molecular line emission in the asymmetric Oph-IRS 48 dust trap: Temperatures, timescales, and sub-thermal excitation

Temmink, M., Booth, A.S., Leemker, M. et al. (8 more authors) (2025) Characterising the molecular line emission in the asymmetric Oph-IRS 48 dust trap: Temperatures, timescales, and sub-thermal excitation. Astronomy & Astrophysics, 693. A101. ISSN 0004-6361

Abstract

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Item Type: Article
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© The Authors 2025. Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Keywords: astrochemistry / protoplanetary disks / stars: variables: T Tauri, Herbig Ae/Be / submillimeter: general
Dates:
  • Published: 7 January 2025
  • Published (online): 7 January 2025
  • Accepted: 18 November 2024
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)
Funding Information:
Funder
Grant number
STFC (Science and Technology Facilities Council)
ST/X001016/1
MRC (Medical Research Council)
MR/T040726/1
Depositing User: Symplectic Publications
Date Deposited: 14 Jan 2025 13:14
Last Modified: 14 Jan 2025 13:14
Status: Published
Publisher: EDP Sciences
Identification Number: 10.1051/0004-6361/202452175
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