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 sev...
Aql X-1 is a soft X-ray transient source and emits type I X-ray bursts. A spectral state transition ...
We have studied the evolution of low-frequency quasi-periodic oscillations (LFQPOs) during the risin...
Aql X-1 is one of the best-studied neutron star low-mass X-ray binaries. It was previously targeted ...
We have obtained I-band photometry of the neutron star X-ray transient Aql X-1 during quiescence. We...
We have obtained I-band photometry of the neutron star X-ray transient Aql X--1 during quiescence. W...
Aql X-1 is the most prolific low-mass X-ray binary transient hosting a neutron star. In this paper w...
We present optical spectroscopy and optical and infrared photometry of the neutron star soft X-ray t...
We searched for coherent X-ray pulsations from Aql X-1 in a series of RXTE observations taken shortl...
We obtained four Chandra/ACIS-S observations beginning two weeks after the end of the November 2000 ...
We present a broad classification of all outbursts detected with the All-Sky Monitor on the Rossi X-...
A number of studies have revealed variability from neutron star low‐mass X‐ray binaries during quies...
We report on the quiescent spectrum measured with Chandra/ACIS-S of the transient, type-I X-ray burs...
We obtained four Chandra/ACIS-S observations beginning 2 weeks after the end of the 2000 November ou...
Aql X-1 is one of the most prolific low-mass X-ray binary transients (LMXBTs) showing outbursts almo...
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Aql X-1 is a soft X-ray transient source and emits type I X-ray bursts. A spectral state transition ...
We have studied the evolution of low-frequency quasi-periodic oscillations (LFQPOs) during the risin...
Aql X-1 is one of the best-studied neutron star low-mass X-ray binaries. It was previously targeted ...
We have obtained I-band photometry of the neutron star X-ray transient Aql X-1 during quiescence. We...
We have obtained I-band photometry of the neutron star X-ray transient Aql X--1 during quiescence. W...
Aql X-1 is the most prolific low-mass X-ray binary transient hosting a neutron star. In this paper w...
We present optical spectroscopy and optical and infrared photometry of the neutron star soft X-ray t...
We searched for coherent X-ray pulsations from Aql X-1 in a series of RXTE observations taken shortl...
We obtained four Chandra/ACIS-S observations beginning two weeks after the end of the November 2000 ...
We present a broad classification of all outbursts detected with the All-Sky Monitor on the Rossi X-...
A number of studies have revealed variability from neutron star low‐mass X‐ray binaries during quies...
We report on the quiescent spectrum measured with Chandra/ACIS-S of the transient, type-I X-ray burs...
We obtained four Chandra/ACIS-S observations beginning 2 weeks after the end of the 2000 November ou...
Aql X-1 is one of the most prolific low-mass X-ray binary transients (LMXBTs) showing outbursts almo...
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Aql X-1 is a soft X-ray transient source and emits type I X-ray bursts. A spectral state transition ...
We have studied the evolution of low-frequency quasi-periodic oscillations (LFQPOs) during the risin...
Aql X-1 is one of the best-studied neutron star low-mass X-ray binaries. It was previously targeted ...