Doyle, AP and Davies, GR and Smalley, B and Chaplin, WJ and Elsworth, Y (2014) Determining stellar macroturbulence using asteroseismic rotational velocities from Kepler. Monthly Notices of the Royal Astronomical Society, 444 (4). 3592 -3602. ISSN 1365-2966

[img]
Preview
Text
MNRAS-2014-Doyle-3592-602.pdf - Published Version

Download (565kB) | Preview
Item Type: Article
Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Uncontrolled Keywords: asteroseismology, line: profiles, planets and satellites: fundamental parameters, stars: rotation
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Faculty of Natural Sciences > School of Physical and Geographical Sciences
Related URLs:
Depositing User: Symplectic
Date Deposited: 14 Jul 2015 13:11
Last Modified: 19 Sep 2017 15:00
URI: http://eprints.keele.ac.uk/id/eprint/716

Actions (login required)

View Item View Item