Photoelectric light curve and period study for RZ Draconis

Details Photoelectric light curve and period study for RZ Draconis Photoelectric light curve and period study for RZ Draconis

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pasp...92..463m&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 92, Aug.-Sept. 1980, p. 463-467.

Astronomy and Astrophysics

Astronomy

4

B Stars, Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Brightness, Electrophotometry, Hertzsprung-Russell Diagram

Scientific paper

Photoelectric observations in V and B are presented. The magnitudes and color indices at the four phases of principal interest are V = 11m.01, (B-V) = 0m.31 at phase 0.0; V = 10m.14, (B-V) = 0m.25 at phase 0.25; V = 10m.38, (B-V) = 0m.25 at phase 0.5; and V = 10m.14, (B-V) = 0m.24 at phase 0.75.
The (0- C) diagram indicates that the orbital period was constant from the time of the star's discovery as a variable in 1907 until about 1968. At that time the period suddenly decreased by about 2.9 × 10-6 days.
The current period is 0d.95508738, and the time of minimum derived from the observations in this paper is JD (hel.) 2444177.5555.

Affiliated with

Also associated with

No associations

Rating

Photoelectric light curve and period study for RZ Draconis 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 Photoelectric light curve and period study for RZ Draconis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photoelectric light curve and period study for RZ Draconis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1275902