Observations of X-Per in optical domain

Details Observations of X-Per in optical domain Observations of X-Per in optical domain

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..95...65s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 95, no. 1, Sept. 1983, p. 65-77.

Astronomy and Astrophysics

Astrophysics

4

B Stars, Binary Stars, Light Curve, Variable Stars, X Ray Sources, Pulsars, Stellar Magnitude, Stellar Oscillations, Ubv Spectra

Scientific paper

The authors have monitored the X-ray source X Per (4U 0352+30) on 31 August, 1979 through a U filter for about 1.5 hr using the 102-cm telescope of Kavalur Observatory. During this period intensity of X Per fluctuated for some time, on time scales of few minutes but recovered in the end. It was again monitored from 27 December, 1979 to January 1980 through a standard U, B, V photometer attached to a 34 cm telescope. In this paper the data on the fast flickerings observed on 31 August, 1979 and on the long term monitoring from December 1979 to January 1980 are presented.

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