Ostensen RH, Degroote P, Telting JH, Vos J, Aerts C, Jeffery CS, Green EM, Reed MD, Heber U (2012)
Publication Type: Journal article
Publication year: 2012
Book Volume: 753
Article Number: L17
Journal Issue: 1
DOI: 10.1088/2041-8205/753/1/L17
We introduce the first g-mode pulsator found to reside on the classical blue horizontal branch. One year of Kepler observations of KIC1718290 reveals a rich spectrum of low-amplitude modes with periods between 1 and 12 hr, most of which follow a regular spacing of 276.3s. This mode structure strongly resembles that of the V1093Her pulsators, with only a slight shift toward longer periods. Our spectroscopy, however, reveals KIC1718290 to be quite distinct from the sdB stars that show V1093Her pulsations, which all have surface gravities higher than log g= 5.1 and helium abundances depleted by at least an order of magnitude relative to the solar composition. We find that KIC1718290 has T
APA:
Ostensen, R.H., Degroote, P., Telting, J.H., Vos, J., Aerts, C., Jeffery, C.S.,... Heber, U. (2012). KIC 1718290: A helium-rich V1093-her-like pulsator on the blue horizontal branch. Astrophysical Journal Letters, 753(1). https://doi.org/10.1088/2041-8205/753/1/L17
MLA:
Ostensen, R. H., et al. "KIC 1718290: A helium-rich V1093-her-like pulsator on the blue horizontal branch." Astrophysical Journal Letters 753.1 (2012).
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