Aql X-1 in Outburst and Quiescence
arXiv:astro-ph/9901075 · doi:10.1086/307283
Abstract
We present photometry and spectroscopy of the soft x-ray transient Aql X-1. Optical photometry during an active state shows a strong (0.6 mag peak-to-peak) modulation at a period of 19 hours. Infrared (K'-band) photometry during a quiescent state limits any ellipsoidal variations to <0.07 mag (peak-to-peak), which implies an inclination i<31 (90% limit). Spectroscopy in a quiescent state shows at most very small radial velocity variations, which implies a very low inclination of i<12 (90% limit). The low inclination is rather unexpected given the large photometric modulation seen in the active state. The upper limit to the equivalent width of the anomalous Li 6707A line is <0.3A, which is similar to the measured strength of this line in several other x-ray transients.
Accepted for publication in ApJ, 12 pages, 5 figures
References in corpus (5)
- Aquila X-1 from outburst to quiescence: the onset of the propeller effect and signs of a turned-on rotation-powered pulsar
- The mass of the neutron star in Cyg X-2 (V1341 Cyg)
- Spectral State Transitions in Aql X-1: Evidence for `Propeller' Effects
- An ``outside-in'' outburst of Aql X--1
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- Variable Thermal Emission from Aql X-1 in Quiescence
- Quiescent Thermal Emission from the Neutron Star in Aql X-1
- The disc-jet coupling in the neutron star X-ray binary Aquila X-1
- The Orbital Light Curve of Aquila X-1
- The evolution of the high energy tail in the quiescent spectrum of the soft X-ray transient Aql X-1
- The donor of Aquila X-1 revealed by high angular resolution near-infrared spectroscopy
- Polarised infrared emission from X-ray binary jets
- Measuring A Truncated Disk in Aquila X-1
- Truncation of the Accretion Disk at One Third of the Eddington Limit in the Neutron Star Low-Mass X-ray Binary Aquila X-1
- An anti-correlation between X-ray luminosity and H-alpha equivalent width in X-ray binaries
- Intermittent dipping in a low-mass X-ray Binary
- A detection of the donor star of Aquila X-1 during its 2004 outburst?
- Serendipitous Discovery of a Cataclysmic Variable in the Globular Cluster NGC 6624
- Lithium enhancement in X-ray binaries due to stellar rotation
- Optical nebular emission following the most luminous outburst of Aquila X-1
- Probing thermonuclear bursts and X-ray reflection features in Aql X-1 during 2024 outburst
- Ubiquitous yet forgotten: broad absorptions in the optical spectra of low-mass X-ray binaries