IGR J01583+6713
Revision as of 13:35, 18 April 2018 by Kuehnel (talk | contribs) (Created page with "Category:Accreting X-ray Pulsars '''Monitoring data''': [http://xte.mit.edu/asmlc/srcs/igrj01583+6713.html RXTE/ASM] = Coordinates = {| class="wikitable" | RA | 01h 5...")
Monitoring data:
RXTE/ASM
Coordinates
| RA | 01h 58m 18.2 s | Dec | +67° 13' 26" |
| RA | 29.575833 | Dec | +67.223889 |
| l | 129.3516 | b | +05.1893 |
Binary system
Porb= ?
Pspin=469.2 s Tentative detection by Swift (et al.(2008)]). Not detected by INTEGRAL [Wang(2010)
Optical companion
The companion star is a B2 IVe at a distance of ~4.0 kpc (Kaur et al.(2008))
E(B-V) = 1.46 mag
Main publications
- Discovery of a magnetic neutron star in X-ray transient IGR J01583+6713 Wang(2010)
- Multiwavelength study of the transient X-ray binary IGR J01583+6713 Kaur et al.(2008)
Spectrum
The 20-100 keV spectrum can be fitted by a bremsstrahlung model of kT ~ 35 keV or a power-law model of Gamma ~ 2.1. In addition, electron resonant cyclotron absorption lines were detected at ~ 35 keV and possibly at 67 keV, implying that a magnetic field of B ~ 4 × 1012 G.