A probable 3.0455-hr period in the outburst light curve of the recurrent nova V404Cyg

Details A probable 3.0455-hr period in the outburst light curve of the recurrent nova V404Cyg A probable 3.0455-hr period in the outburst light curve of the recurrent nova V404Cyg

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.250..385l&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 250, May 15, 1991, p. 385-391. Research supported by Mi

Astronomy and Astrophysics

Astronomy

13

Astronomical Photometry, Light Curve, Novae, Stellar Flares, Power Spectra, Stellar Luminosity, Stellar Magnitude, Temporal Distribution

Scientific paper

Photometric observations of the nova V4O4Cyg have been performed during 1989 May-July, immediately following its recent outburst. Measurements in the R photometric band have revealed periodic variability superposed on the general decline in the brightness of the star by 3 mag during that interval. The amplitude of the cyclic variation decreased from 0.24 mag in May-June, to 0.06 mag in July. A period analysis of the data suggests that the photometric cycle has a period of 3.0455 hr. This may well be the orbital period of the V4O4Cyg binary system.

Affiliated with

Also associated with

No associations

Rating

A probable 3.0455-hr period in the outburst light curve of the recurrent nova V404Cyg does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A probable 3.0455-hr period in the outburst light curve of the recurrent nova V404Cyg, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A probable 3.0455-hr period in the outburst light curve of the recurrent nova V404Cyg will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1038954