Spectro-astrometry of the pre-transitional star LkCa 15 does not reveal an accreting planet but extended H alpha emission

Mendigutía, I, Oudmaijer, RD orcid.org/0000-0001-7703-3992, Schneider, PC et al. (4 more authors) (2018) Spectro-astrometry of the pre-transitional star LkCa 15 does not reveal an accreting planet but extended H alpha emission. Astronomy and Astrophysics, 618. ARTN L9. ISSN 1432-0746

Abstract

Metadata

Authors/Creators:
Copyright, Publisher and Additional Information: © ESO 2018. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: stars: pre-main sequence; protoplanetary disks; stars: individual: LkCa 15; techniques: high angular resolution; techniques: spectroscopic
Dates:
  • Published: 25 October 2018
  • Accepted: 4 October 2018
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds)
Funding Information:
FunderGrant number
PPARCST/F002092/1
Science & Technology Facilities Council (STFC)ST/F002092/1
Science & Technology Facilities Council (STFC)ST/I001557/1
Science & Technology Facilities Council (STFC)ST/I001557/1
Science & Technology Facilities Council (STFC)ST/L000628/1
Science & Technology Facilities Council (STFC)ST/P00041X/1
Depositing User: Symplectic Publications
Date Deposited: 22 Jan 2019 13:53
Last Modified: 12 Jul 2019 15:17
Status: Published
Publisher: EDP Sciences
Identification Number: https://doi.org/10.1051/0004-6361/201834233
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