Timing Analysis of the Intermediate Polar V709 Cas
Srinivas M. Rao,
Aryabhatta Research Institute of observational sciencES (ARIES), Nainital 263001, India. Corresponding author: srinivas22546@gmail.com
Jeewan Chandra Pandey,
Aryabhatta Research Institute of observational sciencES (ARIES), Nainital 263001, India
Nikita Rawat,
Aryabhatta Research Institute of observational sciencES (ARIES), Nainital 263001, India
Arti Joshi,
Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile
Abstract
We have carried detailed time-resolved timing analysis of an intermediate polar V709 Cas, using the long-baseline, short-cadence optical photometric data from the Transiting Exoplanet Survey Satellite. We found an orbital period of 5.3341±0.0004 hr, a spin period of 312.75±0.02 sec, and a beat period of 317.93±0.03 sec, which is similar to the earlier published results. From the continuous high cadence data, we found that V709 Cas is a disc overflow system with disc-fed dominance.
Keywords : Cataclysmic Variable, Intermediate Polars (V709 Cas), Accretion Geometry
Pour citer cet article
Srinivas M. Rao, Jeewan Chandra Pandey, Nikita Rawat & Arti Joshi, «Timing Analysis of the Intermediate Polar V709 Cas», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 93 - Année 2024, No 2 - Proceeedings of the 3rd BINA Workshop on the Scientific Potential of the Indo-Belgian Cooperation, 327-332 URL : http://popups.ulg.be/0037-9565/index.php?id=11698.