Can a Bright and Energetic X-Ray Pulsar Be Hiding Amid the Debris of SN 1987A? (2018)
Attributed to:
Dust formation by supernovae and asymptotic giant branch stars
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aab6b6
Publication URI: http://dx.doi.org/10.3847/1538-4357/aab6b6
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1