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Aquila X-1 in outburst and quiescence

  • Michael R. Garcia
  • , Paul J. Callanan
  • , John McCarthy
  • , Kristoffer Eriksen
  • , Robert M. Hjellming

Research output: Contribution to journalArticlepeer-review

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 languageEnglish
Pages (from-to)422-427
Number of pages6
JournalAstrophysical Journal
Volume518
Issue number1 PART 1
DOIs
Publication statusPublished - 10 Jun 1999

Keywords

  • Binaries: close
  • Stars: individual (Aquila X-1)
  • Stars: neutron
  • X-rays: stars

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