📣 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.

High-mass star formation across the Large Magellanic Cloud I. Chemical properties and hot molecular cores observed with ALMA at 1.2 mm (2024)

First Author: Golshan R

Attributed to: Astrophysics and Cosmology Research at the Jodrell Bank Centre for Astrophysics 2023-2026 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202349077

Publication URI: http://dx.doi.org/10.1051/0004-6361/202349077

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics