"Peremennye Zvezdy",
Prilozhenie,
vol. 8, N 23 (2008)
Prilozhenie,
vol. 8, N 23 (2008)
Light Elements of V671 Ori
A. Samokhvalov
Surgut, Russia
Received: 8.05.2008; accepted: 28.05.2008
(E-mail for contact: sav@surgut.ru)
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Remarks: |
| V671 Ori was discovered as an Algol-type variable
by Hoffmeister (1967). Its orbital period
has
remained unknown until now. The Opical Monitoring Camera (Mas-Hesse et al.,
2003) on board the INTEGRAL spacecraft obtained 620 V-band observations
on JD 2452932 - 2453793. These observations are available via
the OMC Data Server (Gutierrez et al., 2004; https://sdc.laeff.inta.es/omc/secure/form_busqueda.jsp).
We used the Peranso software to determine
the orbital period of the eclipsing system.
Min II = 13.8.
The light elements are: Min = HJD2452932.63 + 0.66334d E. Acknowledgements: This research is based on the data from the OMC Archive at LAEFF, pre-processed by ISDC. The author is grateful to K.V. Sokolovsky for his suggestion to find the period of V671 Ori and to S.V. Antipin for helpful discussion. |
| References: |
| Gutierrez, R., Solano, E., Domingo, A., Garcia, J., 2004, ASP Conference Series,
314, 153
Hoffmeister, C., 1967, AN, 290, 43 Mas-Hesse, J. M., Gimenez, A., Culhane, J.L., et al., 2003, A&A, 411, L261 |
Light Curve
Data Source |