The unique opportunity to determine the mass of an accreting neutron star: the eclipsing accretion powered X-ray pulsar SWIFTJ1749.4-2807 (2014)
Attributed to:
Warwick Astronomy and Astrophysics Rolling Grant 2011-2016
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Type: Working Paper
Parent Publication: NOAO Proposal