Photometric observations of CN Orionis

Details Photometric observations of CN Orionis Photometric observations of CN Orionis

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...115..190s&link_type=abstract

Astronomy and Astrophysics, vol. 115, no. 1, Nov. 1982, p. 190-196. Deutsche Forschungsgemeinschaft

Astronomy and Astrophysics

Astrophysics

21

Astronomical Photometry, Binary Stars, Dwarf Novae, Light Curve, Stellar Models, Variable Stars, Bursts, Mass Transfer, Orbital Elements, Orion Constellation

Scientific paper

Extended photometric observations of CN Ori have been carried out in December 1981 during 14 of 16 consecutive nights. Two eruptions and the minimum stage in between were covered. The lightcurves show humplike variations with two periods of 0.1631 d and 0.1595 d, the longer one being the orbital period. The amplitude of the orbital hump does not vary considerably during the observations. This is shown to be an argument in favor of the Osaki model for dwarf nova outbursts. System parameters of CN Ori are estimated using the orbital period and high frequency oscillation periods.

Affiliated with

Also associated with

No associations

Rating

Photometric observations of CN Orionis 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 Photometric observations of CN Orionis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometric observations of CN Orionis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1755150