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Periodicities in the K2 light curve of HP Librae

Solanki, Siddhant; Kupfer, Thomas; Blaes, Omer; Breedt, Elmé; Scaringi, Simone

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Authors

Siddhant Solanki

Thomas Kupfer

Omer Blaes

Elmé Breedt



Abstract

We analyse Kepler/K2 light-curve data of the AM CVn system HP Librae (HP Lib). We detect with confidence four photometric periodicities in the system: the orbital frequency, both positive and negative superhumps, and the positive apsidal precession frequency of the accretion disc. This is only the second time that the apsidal precession frequency has ever been directly detected in the photometry of a helium accreting system, after SDSS J135154.46-064309.0. We present phase-folded light curves and sliding power spectra of each of the four periodicities. We measure rates of change of the positive superhump period of ∼10−7 d. We also redetect a quasi-periodic oscillation (QPO) at ∼300 cyc d–1, a feature that has been stable over decades, and show that it is harmonically related to two other QPOs, the lowest of which is centred on the superhump/orbital frequency. The continuum power spectrum is consistent with a single power law with no evidence of any breaks within our observed frequency range.

Citation

Solanki, S., Kupfer, T., Blaes, O., Breedt, E., & Scaringi, S. (2021). Periodicities in the K2 light curve of HP Librae. Monthly Notices of the Royal Astronomical Society, 500(1), 1222-1230. https://doi.org/10.1093/mnras/staa3240

Journal Article Type Article
Acceptance Date Oct 15, 2020
Online Publication Date Oct 20, 2020
Publication Date 2021-01
Deposit Date Dec 31, 2020
Publicly Available Date Jun 29, 2021
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 500
Issue 1
Pages 1222-1230
DOI https://doi.org/10.1093/mnras/staa3240

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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2020 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.





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