Timing Analysis of the Intermediate Polar V709 Cas

Fuente: arXiv
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Autores principales: Rao, Srinivas M, Pandey, Jeewan Chandra, Rawat, Nikita, Joshi, Arti
Formato: Preprint
Publicado: 2023
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author Rao, Srinivas M
Pandey, Jeewan Chandra
Rawat, Nikita
Joshi, Arti
author_facet Rao, Srinivas M
Pandey, Jeewan Chandra
Rawat, Nikita
Joshi, Arti
contents 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 $\pm$ 0.0004 hr, a spin period of 312.75 $\pm$ 0.02 sec, and a beat period of 317.93 $\pm$ 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.
format Preprint
id arxiv_https___arxiv_org_abs_2309_03150
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Timing Analysis of the Intermediate Polar V709 Cas
Rao, Srinivas M
Pandey, Jeewan Chandra
Rawat, Nikita
Joshi, Arti
Solar and Stellar Astrophysics
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 $\pm$ 0.0004 hr, a spin period of 312.75 $\pm$ 0.02 sec, and a beat period of 317.93 $\pm$ 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.
title Timing Analysis of the Intermediate Polar V709 Cas
topic Solar and Stellar Astrophysics
url https://arxiv.org/abs/2309.03150