no code implementations • 18 Jan 2021 • C. Malacaria, P. Kretschmar, K. K. Madsen, C. A. Wilson-Hodge, Joel B. Coley, P. Jenke, A. A. Lutovinov, K. Pottschmidt, S. S. Tsygankov, J. Wilms
Accreting X-ray pulsars (XRPs) undergo luminous X-ray outbursts during which the spectral and timing behavior of the neutron star can be studied in detail.
High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
1 code implementation • 9 Oct 2019 • V. Morello, E. F. Keane, T. Enoto, S. Guillot, W. C. G. Ho, A. Jameson, M. Kramer, B. W. Stappers, M. Bailes, E. D. Barr, S. Bhandari, M. Caleb, C. M. L. Flynn, F. Jankowski, S. Johnston, W. van Straten, Z. Arzoumanian, S. Bogdanov, K. C. Gendreau, C. Malacaria, P. S. Ray, R. A. Remillard
We report the discovery of PSR J2251$-$3711, a radio pulsar with a spin period of 12. 1 seconds, the second longest currently known.
High Energy Astrophysical Phenomena