A Strong Emission Line near 24.8 Å in the X-Ray Binary System MAXI J0556-332: Gravitational Redshift or Unusual Donor?
Article
Publications
Complete Citation
- Maitra, Dipankar, Miller, Jon M., Raymond, John C., and Reynolds, Mark T. 2011. "A Strong Emission Line near 24.8 Å in the X-Ray Binary System MAXI J0556-332: Gravitational Redshift or Unusual Donor?" The Astrophysical Journal Letters, 743, (1). https://doi.org/10.1088/2041-8205/743/1/L11.
Overview
Abstract
- We report the discovery of a strong emission line near 24.8 Å (0.5 keV) in the newly discovered X-ray binary system MAXI J0556-332 with the reflection grating spectrometer (RGS) on board the XMM-Newton observatory. The X-ray light curve morphology during these observations
Publication Date
- 2011
