Orbital period changes in RW CrA, DX Vel and V0646 Cen

Rok, strany: 2017, 29 - 52

We aim to determine the absolute parameters of the components of southern Algol-type binaries with deep eclipses RW CrA, DX Vel, V0646 Cen and interpret their orbital period changes. The data analysis is based on a high quality Walraven photoelectric photometry, obtained in the 1960-70s, our recent CCD photometry, ASAS (Pojmanski, 2002), and Hipparcos (Perryman et al., 1997) photometry of the objects. Their light curves were analyzed using the PHOEBE program with fixed effective temperatures of the primary components, found from disentangling the Walraven (B-U) and (V-B) colour indices. We found the absolute parameters of the components of all three objects. All reliable observed times of minimum light were used to construct and analyze the Eclipse Time Variation (ETV) diagrams. We interpreted the ETV diagrams of the detached binary RW CrA and the semi-detached binary DX Vel by a LIght-Time Effect (LITE), estimated parameters of their orbits and masses of their third bodies. We suggest a long term variation of the inclination angle of both eclipsing binaries, caused by a non-coplanar orientation of their third body orbits. We interpreted the detected orbital period increase in the semi-detached binary V0646 Cen by a mass transfer from the less to more massive component with the rate Ṁ = 6.08×10^-9 M_☉/yr.

ISO 690:

Volkov, I., Chochol, D., Grygar, J., Mašek, M., Juryšek, J. 2017. Orbital period changes in RW CrA, DX Vel and V0646 Cen. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 47, no.1, pp. 29-52. 1335-1842.

APA:

Volkov, I., Chochol, D., Grygar, J., Mašek, M., Juryšek, J. (2017). Orbital period changes in RW CrA, DX Vel and V0646 Cen. Contributions of the Astronomical Observatory Skalnaté Pleso, 47(1), 29-52. 1335-1842.