| Name: | Srinivas M Rao |
| Affiliation: | Aryabhatta Reasearch Institute of Observational Sciences, Nainital |
| Conference ID : | ASI2023_277 |
| Title : | Change in accretion flow in an Intermediate Polar V709 Cas |
| Authors : | Srinivas M Rao, Jeewan C. Pandey, Nikita Rawat, Arti Joshi |
| Mode of Presentation: | Poster |
| Abstract Category : | Stars, ISM and Galaxy |
| Abstract : | We have carried out 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(TESS). We found an orbital period of 5.33306 ± 0.00004 hr, a spin period of 312.748 ± 0.002 sec and a beat period of 317.927 ± 0.002 sec, which are similar but more precise than the earlier published results. From the continuous data, we report the system’s accretion geometry as disc overflow with disc-fed dominance. The double-peaked pulse profile nature shows it being a two-pole accretor. |
