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19 April 2024 |
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XTE J1946+274 = GRO J1944+26: An Enigmatic Be/X-ray Binary | | Colleen. A. Wilson
; Mark. H. Finger
; M.J. Coe
; Ignacio Negueruela
; | | Date: |
6 Nov 2002 | | Journal: | Astrophys.J. 584 (2003) 996-1007 | | Subject: | astro-ph | | Affiliation: | NSSTC), M.J. Coe (Southampton), Ignacio Negueruela (Strasbourg | | Abstract: | XTE J1946+274 = GRO J1944+26 is a 15.8 s Be/X-ray pulsar discovered simultaneously in 1998 September with the Burst and Transient Source Experiment (BATSE) on the Compton Gamma Ray Observatory (CGRO) and the All-Sky Monitor (ASM) on the Rossi X-ray Timing Explorer (RXTE). Here we present new results from BATSE and {em RXTE} including a pulse timing analysis, spectral analysis, and evidence for an accretion disk. Our pulse timing analysis yielded an orbital period of 169.2 days, a moderate eccentricity of 0.33, and implied a mass function of 9.7 M_sun. We observed evidence for an accretion disk, a correlation between measured spin-up rate and flux, which was fitted to obtain a distance estimate of 9.5 +/- 2.9 kpc. XTE J1946+274 remained active from 1998 September - 2001 July, undergoing 13 outbursts that were not locked in orbital phase. Comparing RXTE PCA observations from the initial bright outburst in 1998 and the last pair of outbursts in 2001, we found energy and intensity dependent pulse profile variations in both outbursts and hardening spectra with increasing intensity during the fainter 2001 outbursts. In 2001 July, optical Halpha observations indicate a density perturbation appeared in the Be disk as the X-ray outbursts ceased. We propose that the equatorial plane of the Be star is inclined with respect to the orbital plane in this system and that this inclination may be a factor in the unusual outburst behavior of the system. | | Source: | arXiv, astro-ph/0211124 | | Services: | Forum | Review | PDF | Favorites | |
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