UBV photometry of DX Aquarii

Details UBV photometry of DX Aquarii UBV photometry of DX Aquarii

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.111..225s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 111, no. 2, April 1985, p. 225-236.

Astronomy and Astrophysics

Astrophysics

4

Eclipsing Binary Stars, Light Curve, Stellar Motions, Stellar Spectrophotometry, Ubv Spectra, Minima, Stellar Color, Stellar Luminosity, Stellar Magnitude, Stellar Occultation, Stellar Orbits, Variable Stars

Scientific paper

U, B, V photometry of the eclipsing binary DX Aqr is presented. The period of the system comes out to be nearly half the period given by Strohmeier (1966) and a value of 0.472502 d is determined. The color of the system is discussed. It is shown that the primary eclipse is a total occultation, that the orbit seems to be eccentric, and that the system belongs to Algol type. DX Aqr may be a very complicated system. The present results are considerably different from those of earlier investigations by Strohmeier et al. (1965), Strohmeier (1966), Cowley et al. (1969), and Olsen (1976).

Affiliated with

Also associated with

No associations

Rating

UBV photometry of DX Aquarii 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 UBV photometry of DX Aquarii, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UBV photometry of DX Aquarii will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1288491