GX 1+4 : pulse period measurement and detection of phase-variable iron line emission.
Abstract
Observations of the X-ray source GX 1+4 (1728 - 247) made by Ariel 6 in 1979 July and 1980 April show that the pulse period decreased at a faster rate during 1978-80 than over the period 1970-78. Compared with that measured in 1976, the pulse profile had become more sinusoidal, with an apparent phase lag of 0.1 between the 4-8 keV pulse and that seen at energies above 25 keV. The 1-4 keV range does not show pulsations and is stronger than hitherto. There is also an iron emission feature whose equivalent width varies with pulse phase.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- November 1982
- DOI:
- Bibcode:
- 1982MNRAS.201..759R
- Keywords:
-
- Emission Spectra;
- Iron;
- Line Spectra;
- Pulse Duration;
- Stellar Spectra;
- X Ray Sources;
- Abundance;
- Ariel Satellites;
- Fluorescence;
- Sine Waves;
- Spectral Line Width;
- X Ray Astronomy;
- Astronomy