Optical and Infrared Photometry of the Microquasar GRO J1655−40 in Quiescence
Open Access
- 20 June 2001
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 554 (2), 1290-1297
- https://doi.org/10.1086/321411
Abstract
We present BVIJK photometry of the black hole candidate GRO J1655-40 in full quiescence. We report a refined orbital period of 2.62191 ± 0.00020 days. The light curves are dominated by ellipsoidal variations from the secondary star. We model the light curves with an upgraded code that includes a more accurate treatment of limb darkening. Previous models containing a large cool disk are ruled out, and, indeed, our data can be fitted with a pure ellipsoidal light curve without any disk contribution. In general agreement with previous results, we derive a confidence region of the correlated quantities inclination and mass ratio, centered on an inclination of 702 ± 19 and mass ratio of 2.6 ± 0.3, resulting in a primary mass M1 = 6.3 ± 0.5 M☉ (all 95% confidence). The complex limits and errors on these values and on the possible disk contribution to the light curve are discussed.This publication has 21 references indexed in Scilit:
- TheNextGenModel Atmosphere Grid. II. Spherically Symmetric Model Atmospheres for Giant Stars with Effective Temperatures between 3000 and 6800 KThe Astrophysical Journal, 1999
- Evidence of a supernova origin for the black hole in the system GRO J1655 - 40Nature, 1999
- The Mass Distribution of Stellar Black HolesThe Astrophysical Journal, 1998
- Optical Observations of GRO J1655−40 in Quiescence. I. A Precise Mass for the Black Hole PrimaryThe Astrophysical Journal, 1997
- A New Model for Black Hole Soft X-Ray Transients in QuiescenceThe Astrophysical Journal, 1996
- Dynamical evidence for a black hole in the eclipsing X-ray nova GRO J1655 – 40Nature, 1995
- Spectroscopy of Formula: the mass of the black hole and an image of its accretion discMonthly Notices of the Royal Astronomical Society, 1994
- THE LIMIT CYCLE INSTABILITY IN DWARF NOVA ACCRETION DISKSThe Chaotic Universe, 1993
- Approximations to the radii of Roche lobesThe Astrophysical Journal, 1983
- Stationary configurations and the upper bound on the mass of nonrotating, causal neutron starsThe Astrophysical Journal, 1976