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Article overview
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Kepler's first view of O-star variability: K2 data of five O stars in Campaign 0 as a proof-of-concept for O-star asteroseismology | B. Buysschaert
; C. Aerts
; S. Bloemen
; J. Debosscher
; C. Neiner
; M. Briquet
; J. Vos
; P. Papics
; R. Manick
; V. Schmid
; H. Van Winkel
; A. Tkachenko
; | Date: |
11 Jul 2015 | Abstract: | We present high-precision photometric light curves of five O-type stars
observed with the refurbished {it Kepler/} satellite during its Campaign 0.
For one of the stars, we also assembled high-resolution ground-based
spectroscopy with the {sc hermes} spectrograph attached to the 1.2-m Mercator
telescope. The stars EPIC202060097 (O9.5V) and EPIC202060098 (O7V) exhibit
monoperiodic variability due to rotational modulation with an amplitude of 5.6
mmag and 9.3 mmag and a rotation period of 2.63 d and 5.03 d, respectively.
EPIC202060091 (O9V) and EPIC202060093 (O9V:pe) reveal variability at low
frequency but the cause is unclear. EPIC202060092 (O9V:p) is discovered to be a
spectroscopic binary with at least one multiperiodic $eta,$Cep-type pulsator
whose detected mode frequencies occur in the range $[0.11,6.99]$ d$^{-1}$ and
have amplitudes between 0.8 and 2.0 mmag. Its pulsation spectrum is shown to be
fully compatible with the ones predicted by core-hydrogen burning O-star
models. Despite the short duration of some 33,d and the limited data quality
with a precision near 100 $mu$mag of these first K2 data, the diversity of
possible causes for O-star variability already revealed from campaigns of
similar duration by the MOST and CoRoT satellites is confirmed with {it
Kepler}. We provide an overview of O-star space photometry and give arguments
why future K2 monitoring during Campaigns 11 and 13 at short cadence,
accompanied by time-resolved high-precision high-resolution spectroscopy opens
up the possibility of in-depth O-star seismology. | Source: | arXiv, 1507.3091 | Services: | Forum | Review | PDF | Favorites |
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