The microquasar XTE J1807-294 - Mass evaluation by means of the relativistic precession model
Abstract
The high frequency quasiperiodic oscillations (QPOs) in the X-ray spectra of the millisecond pulsar XTE J1807-294 are under consideration. By application of the relativistic precession (RP) model an attempt is made to approximate the observed frequencies as well as to assess the mass and the angular momentum of the object. The obtained mass is too high for a neutron star.
- Publication:
-
10th Jubilee International Conference of the Balkan Physical Union
- Pub Date:
- February 2019
- DOI:
- 10.1063/1.5091221
- Bibcode:
- 2019AIPC.2075i0007T