CaltechAUTHORS
  A Caltech Library Service

KIC 8164262: a heartbeat star showing tidally induced pulsations with resonant locking

Hambleton, K. and Fuller, J. and Thompson, S. and Prša, A. and Kurtz, D. W. and Shporer, A. and Isaacson, H. and Howard, A. W. and Endl, M. and Cochran, W. and Murphy, S. J. (2018) KIC 8164262: a heartbeat star showing tidally induced pulsations with resonant locking. Monthly Notices of the Royal Astronomical Society, 473 (4). pp. 5165-5176. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:20180221-154459222

[img] PDF - Published Version
See Usage Policy.

1423Kb
[img] PDF - Submitted Version
See Usage Policy.

1527Kb

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20180221-154459222

Abstract

We present the analysis of KIC 8164262, a heartbeat star with a high-amplitude (∼1 mmag), tidally resonant pulsation (a mode in resonance with the orbit) at 229 times the orbital frequency and a plethora of tidally induced g-mode pulsations (modes excited by the orbit). The analysis combines Kepler light curves with follow-up spectroscopic data from the Keck telescope, KPNO (Kitt Peak National Observatory) 4-m Mayall telescope and the 2.7-m telescope at the McDonald observatory. We apply the binary modelling software, PHOEBE, to the Kepler light curve and radial velocity data to determine a detailed binary star model that includes the prominent pulsation and Doppler boosting, alongside the usual attributes of a binary star model (including tidal distortion and reflection). The results show that the system contains a slightly evolved F star with an M secondary companion in a highly eccentric orbit (e = 0.886). We use the results of the binary star model in a companion paper (Fuller) where we show that the prominent pulsation can be explained by a tidally excited oscillation mode held near resonance by a resonance locking mechanism.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/stx2673DOIArticle
https://academic.oup.com/mnras/article/473/4/5165/4553530PublisherArticle
https://arxiv.org/abs/1706.05051arXivDiscussion Paper
ORCID:
AuthorORCID
Fuller, J.0000-0002-4544-0750
Thompson, S.0000-0001-7106-4683
Shporer, A.0000-0002-1836-3120
Isaacson, H.0000-0002-0531-1073
Howard, A. W.0000-0001-8638-0320
Endl, M.0000-0002-7714-6310
Cochran, W.0000-0001-9662-3496
Additional Information:© 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2017 October 11. Received 2017 October 11; in original form 2017 June 14. Published: 13 October 2017. The authors express their sincere thanks to NASA and the Kepler team for the high quality Kepler data. The Kepler mission is funded by NASA's Science Mission Directorate. We thank the Planet Hunters for finding this object and Professor Dan Fabrycky for notifying us about it. This work was also supported by the STFC (Science and Technology Funding Council). KH, ST and JF acknowledge support through NASA K2 GO grant (11-KEPLER11-0056) and NASA ADAP grant (16-ADAP16-0201). AP and KH acknowledge support from the NSF (grant #1517460). JF acknowledges partial support from NSF under grant nos. AST-1205732, PHY-1125915 and through a Lee DuBridge Fellowship at Caltech. We would like to thank the RAS for providing grants which enabled KH's attendance to conferences and thus enabled the development of collaborations and the successful completion of this work. AP acknowledges support through NASA K2 GO grant (NASA 14-K2GO1_2-0057). We acknowledge the observations taken using the 4-m Mayall telescope, KPNO (NOAO 2011A-0022); the Keck telescope, Mauna Kea and the 2.7-m telescope at the McDonald Observatory. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts.
Group:TAPIR, Walter Burke Institute for Theoretical Physics
Funders:
Funding AgencyGrant Number
Science and Technology Facilities Council (STFC)UNSPECIFIED
NASA11-KEPLER11-0056
NASA16-ADAP16-0201
NSFAST-1517460
NSFAST-1205732
NSFPHY-1125915
Lee DuBridge Fellowship, CaltechUNSPECIFIED
NASA14-K2GO1_2-0057
NASANAS5-26555
NASANNX09AF08G
Subject Keywords:asteroseismology – binaries: close – binaries: general – stars: individual (KIC 8164262) – stars: oscillations – stars: variables: general
Record Number:CaltechAUTHORS:20180221-154459222
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20180221-154459222
Official Citation:K. Hambleton, J. Fuller, S. Thompson, A. Prša, D. W. Kurtz, A. Shporer, H. Isaacson, A. W. Howard, M. Endl, W. Cochran, S. J. Murphy; KIC 8164262: a heartbeat star showing tidally induced pulsations with resonant locking, Monthly Notices of the Royal Astronomical Society, Volume 473, Issue 4, 1 February 2018, Pages 5165–5176, https://doi.org/10.1093/mnras/stx2673
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:84912
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:22 Feb 2018 18:07
Last Modified:25 Apr 2019 22:36

Repository Staff Only: item control page