Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aj....114.2145m&link_type=abstract
Astronomical Journal v.114, p.2145
Astronomy and Astrophysics
Astronomy
6
Stars: Individual: Rz Tauri, Binaries: Close
Scientific paper
New photometric uvby light curves of the W UMa star RZ Tauri have been obtained, and the differential-corrections method of Wilson and Devinney was used to compute a new set of system parameters. RZ Tauri is confirmed as an over-contact system with q=0.3563 and i81.54°, generating total-annular eclipses. The gravity darkening g=0.83±0.07 places this system between convective and radiative behavior, appropriate for its F0 spectral type. The bolometric albedo A=0.25±0.28 is low, but poorly determined. These light curves were combined with previously-published times of minima to derive a new, quadratic ephemeris, and a previously-published radial-velocity curve was used to determine the mass of the system.
Morris Steven L.
Naftilan Stephen A.
No associations
LandOfFree
RZ Tauri: New Light Curves and Analysis 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 RZ Tauri: New Light Curves and Analysis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and RZ Tauri: New Light Curves and Analysis will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1684762