On the Question of the Behavior of O-C Residuals of the Active Algol-Like Binary RZ Cassiopeiae
| dc.creator | Golovin, Alex | |
| dc.creator | Pavlenko, Elena | |
| dc.date | 2005-11-08 | |
| dc.date.accessioned | 2026-07-07T10:27:42Z | |
| dc.date.available | 2026-07-07T10:27:42Z | |
| dc.description | We present an analysis of the RZ Cassiopeia O-C diagram for a 30-year period, based on data published by the AAVSO. The new parabolic light-elements are determined and P-dot was estimated. This enabled us to establish the value of M-dot, the rate of the mass transfer between components of this eclipsing binary. Deviations from the parabola in the RZ Cas O-C diagram have a wavelike trend. The pulsation of the primary component influences the scatter of O-C points, as well as it influences the shape of the eclipse. Some physical points on such O-C behavior are presented. | |
| dc.description | Accepted to JAAVSO vol. 34 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0511213 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0511213 | |
| dc.identifier | J.Am.Assoc.Var.StarObs.34:46,2005 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/177228 | |
| dc.subject | Astrophysics | |
| dc.title | On the Question of the Behavior of O-C Residuals of the Active Algol-Like Binary RZ Cassiopeiae | |
| dc.type | text |