Cygnus X-1 : optical variation on the 294 day X-ray period.
Abstract
The recently discovered 294 day X-ray period has optical counterparts. A 10 yr B band photometric record shows synchronous changes of 0.01 mag amplitude, with minima coinciding with the X-ray minima. Stronger and weaker variations, respectively, are seen in U and V. The 5.6 day orbital light curves, additionally, show pronounced changes on the 294 day cycle. There is also a 294 day polarization variation.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- August 1983
- DOI:
- 10.1086/184096
- Bibcode:
- 1983ApJ...271L..65K
- Keywords:
-
- Binary Stars;
- Cygnus Constellation;
- Light Curve;
- Ubv Spectra;
- X Ray Sources;
- Orbital Elements;
- Polarization Characteristics;
- Astrophysics