Abstract
We present photometry and spectroscopy of the soft X-ray transient AqI X-1 . Optical photometry during an active state shows a strong (0.6 mag peak-to-peak) modulation at a period of 19 hr. Infrared (K′ band) photometry during a quiescent state limits any ellipsoidal variations to less than 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 6707 A line is less than 0.3 Å, which is similar to the measured strength of this line in several other X-ray transients.
| Original language | English |
|---|---|
| Pages (from-to) | 422-427 |
| Number of pages | 6 |
| Journal | Astrophysical Journal |
| Volume | 518 |
| Issue number | 1 PART 1 |
| DOIs | |
| Publication status | Published - 10 Jun 1999 |
Keywords
- Binaries: close
- Stars: individual (Aquila X-1)
- Stars: neutron
- X-rays: stars
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