The peculiar dipping events in the disc-bearing young-stellar object EPIC 204278916
Abstract
EPIC 204278916 has been serendipitously discovered from its K2 light curve that displays irregular dimmings of up to 65 per cent for ≈25 consecutive days out of 78.8 d of observations. For the remaining duration of the observations, the variability is highly periodic and attributed to stellar rotation. The star is a young, low-mass (M-type) pre-main-sequence star with clear evidence of a resolved tilted disc from Atacama Large Millimeter/submillimeter Array (ALMA) observations. We examine the K2 light curve in detail and hypothesize that the irregular dimmings are caused by either a warped inner disc edge or transiting cometary-like objects in either circular or eccentric orbits. The explanations discussed here are particularly relevant for other recently discovered young objects with similar absorption dips.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- December 2016
- DOI:
- 10.1093/mnras/stw2155
- arXiv:
- arXiv:1608.07291
- Bibcode:
- 2016MNRAS.463.2265S
- Keywords:
-
- comets: general;
- planets and satellites: dynamical evolution and stability;
- stars: early-type;
- stars: individual: (EPIC 204278916);
- stars: peculiar;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- 9 pages, 10 figures. Accepted for publication in MNRAS