Speaker
Dorota Skowron
(Astronomical Observatory, University of Warsaw)
Description
We use radial velocity curves of Long Period Variables from the Gaia
Focused Product Release and match them with optical light curves from
the ASAS-SN project to investigate differences between the phase of
minimum light and the phase of minimum radial velocity. For LSPs, we
find a mean phase offset of -0.18 $\pm$ 0.09 (in phase [0, 1]) between
the radial velocity and light curves, consistent with previous studies
and very similar to that of Mira stars. We also show the phase offsets
for other types of Long Period Variables.
Author
Dorota Skowron
(Astronomical Observatory, University of Warsaw)
Co-authors
Patryk Iwanek
(Astronomical Observatory, University of Warsaw)
Dr
Piotr Kołaczek-Szymański
(Astronomical Observatory, University of Warsaw)