Gaia17biu/SN 2017egm in NGC 3191: The Closest Hydrogen-poor Superluminous Supernova to Date Is in a "Normal," Massive, Metal-rich Spiral Galaxy (2018)
Attributed to:
Astrophysics and Cosmology Research within the JBCA 2017-2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aaa298
Publication URI: http://dx.doi.org/10.3847/1538-4357/aaa298
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1