📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! If you would be interested in being interviewed about the improvements we're making and to have your say about how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community, please email gateway@ukri.org.

Characterising the molecular line emission in the asymmetric Oph-IRS 48 dust trap: Temperatures, timescales, and sub-thermal excitation (2025)

First Author: Temmink M
Attributed to:  Seeding life on habitable planets funded by UKRI FLF

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202452175

Publication URI: http://dx.doi.org/10.1051/0004-6361/202452175

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics