The rotation of low mass stars at 30 Myr in the cluster NGC 3766. (2019)
Attributed to:
Astrophysics at Oxford 2016-2019
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1017/s1743921319009797
PubMed Identifier: 33014118
Publication URI: http://europepmc.org/abstract/MED/33014118
Type: Journal Article/Review
Volume: 15
Parent Publication: Proceedings of the International Astronomical Union. International Astronomical Union
Issue: Suppl 354
ISSN: 1743-9213