|Author||Bord, D. J. ♦ Mook, D. E. ♦ Petro, L. ♦ Hiltner, W. A.|
|Source||United States Department of Energy Office of Scientific and Technical Information|
|Publisher||Institute of Physics (IOP)|
|Subject Keyword||Physics (Astrophysics & Cosmology)-Stars ♦ Physics (Astrophysics & Cosmology)-Quasi-stellar, Radio & X-Ray Sources ♦ Physics Research-Astrophysics & Cosmology-Stars ♦ COSMIC X-RAY SOURCES- VARIATIONS ♦ VARIABLE STARS- VISIBLE RADIATION ♦ LUMINOSITY ♦ PHOTOMETRY ♦ X RADIATION|
|Abstract||UBV photometry of WRA 977 on 36 nights between January and July 1974 reveals activity on a time scale of days at the 0.1 mag level; no activity greater than approx.0.01 mag is observed on a time scale of minutes. Correlogram and periodogram analyses of the light curve reveal no persistent periodic variations of significant amplitude. (AIP)|
|Learning Resource Type||Article|
|Publisher Department||Department of Physics and Astronomy, Dartmouth College|
|Publisher Place||United States|
|Organization||Department of Physics and Astronomy, Dartmouth College|
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