An Examination of the High Amplitude delta Scuti V2455 Cygni
Abstract
We have monitored the pulsating High Amplitude delta Scuti star, V2455 Cyg, for 8 years using spectroscopic and photometric observations. During that time we have noted a number of interesting changes in the light curve that could be associated with a companion or might be intrinsic to the star. We will present radial velocity measurements, photometric light curves, and H-alpha/H-beta observations for this system. We will also explore the potential interpretations of that data.
- Publication:
-
American Astronomical Society Meeting Abstracts #231
- Pub Date:
- January 2018
- Bibcode:
- 2018AAS...23114605H