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A Transient Transit Signature Associated with the Young Star RIK-210

David, Trevor J.; Petigura, Erik A.; Hillenbrand, Lynne A.; Cody, Ann Marie; Cameron, Andrew Collier; Stauffer, John R.; Fulton, B. J.; Isaacson, Howard T.; Howard, Andrew W.; Howell, Steve B.; Everett, Mark E.; Wang, Ji; Benneke, Björn; Hellier, Coel; West, Richard G.; Pollacco, Don; Anderson, David R.

Authors

Trevor J. David

Erik A. Petigura

Lynne A. Hillenbrand

Ann Marie Cody

Andrew Collier Cameron

John R. Stauffer

B. J. Fulton

Howard T. Isaacson

Andrew W. Howard

Steve B. Howell

Mark E. Everett

Ji Wang

Björn Benneke

Richard G. West

Don Pollacco

David R. Anderson



Abstract

We find transient transit-like dimming events within the K2 time series photometry of the young star RIK-210 in the Upper Scorpius OB association. These dimming events are variable in depth, duration, and morphology. High spatial resolution imaging revealed that the star is single and radial velocity monitoring indicated that the dimming events cannot be due to an eclipsing stellar or brown dwarf companion. Archival and follow-up photometry suggest the dimming events are transient in nature. The variable morphology of the dimming events suggests they are not due to a single spherical body. The ingress of each dimming event is always shallower than egress, as one would expect for an orbiting body with a leading tail. The dimming events are periodic and synchronous with the stellar rotation. However, we argue it is unlikely the dimming events could be attributed to anything on the stellar surface based on the observed depths and durations. Variable obscuration by a protoplanetary disk is unlikely on the basis that the star is not actively accreting and lacks the infrared excess associated with an inner disk. Rather, we explore the possibilities that the dimming events are due to magnetospheric clouds, a transiting protoplanet surrounded by circumplanetary dust and debris, eccentric orbiting bodies undergoing periodic tidal disruption, or an extended field of dust or debris near the corotation radius.

Citation

David, T. J., Petigura, E. A., Hillenbrand, L. A., Cody, A. M., Cameron, A. C., Stauffer, J. R., …Anderson, D. R. A Transient Transit Signature Associated with the Young Star RIK-210. Astrophysical Journal, 835(2), 168. https://doi.org/10.3847/1538-4357/835/2/168

Journal Article Type Article
Online Publication Date Jan 27, 2017
Deposit Date May 30, 2023
Journal The Astrophysical Journal
Print ISSN 0004-637X
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 835
Issue 2
Pages 168
DOI https://doi.org/10.3847/1538-4357/835/2/168
Keywords Space and Planetary Science; Astronomy and Astrophysics
Additional Information Journal title: The Astrophysical Journal; Article type: paper; Article title: A Transient Transit Signature Associated with the Young Star RIK-210; Copyright information: © 2017. The American Astronomical Society. All rights reserved.; Date received: 2016-10-18; Date accepted: 2016-12-09; Online publication date: 2017-01-27