CCD Photometry of W UMa Type Binary TY UMa

Details CCD Photometry of W UMa Type Binary TY UMa CCD Photometry of W UMa Type Binary TY UMa

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001jass...18...55k&link_type=abstract

Journal of Astronomy and Space Sciences, vol. 18, no. 1, p. 55-62

Astronomy and Astrophysics

Astronomy

Stars, Binary Stars, Star Spot

Scientific paper

We present VRI CCD photometry of W UMa type binary TY UMa. The light curves show that the secondary minimum is deeper than theprimary minimum and the maximum I (0.p25) is 0.m023 brighter than the maximum II (0.p75). The V light curve has beenanalyzed and the photometric solutions have been determined by the method of Wilson & Devinney differential correction. Weadopted the spot model to explain the asymetric light curve.

Affiliated with

Also associated with

No associations

Rating

CCD Photometry of W UMa Type Binary TY UMa 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 CCD Photometry of W UMa Type Binary TY UMa, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CCD Photometry of W UMa Type Binary TY UMa will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1133497