4.7 Article

The peculiar dipping events in the disc-bearing young-stellar object EPIC 204278916

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 463, Issue 2, Pages 2265-2272

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stw2155

Keywords

comets: general; planets and satellites: dynamical evolution and stability; stars: early-type; stars: individual: (EPIC 204278916); stars: peculiar

Funding

  1. Alexander von Humboldt Foundation
  2. ESA
  3. NASA Science Mission Directorate
  4. NASA [NAS5-26555]
  5. NASA Office of Space Science [NNX13AC07G]
  6. National Science Foundation [DGE-1144469]

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EPIC 204278916 has been serendipitously discovered from its K2 light curve that displays irregular dimmings of up to 65 per cent for approximate to 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.

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