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The excitation of solar-like oscillations in a delta Sct star by efficient envelope convection

Title
The excitation of solar-like oscillations in a delta Sct star by efficient envelope convection
Type
Article in International Scientific Journal
Year
2011
Authors
Antoci, V
(Author)
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Handler, G
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Campante, TL
(Author)
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Thygesen, AO
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Moya, A
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Kallinger, T
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Stello, D
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Grigahcene, A
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Kjeldsen, H
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Bedding, TR
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Lueftinger, T
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Christensen Dalsgaard, J
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Catanzaro, G
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Frasca, A
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De Cat, P
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Uytterhoeven, K
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Bruntt, H
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Houdek, G
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Kurtz, DW
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Lenz, P
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Kaiser, A
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Van Cleve, J
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Allen, C
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Clarke, BD
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Journal
Title: NatureImported from Authenticus Search for Journal Publications
Vol. 477
Pages: 570-573
ISSN: 0028-0836
Publisher: Springer Nature
Other information
Authenticus ID: P-002-MF8
Abstract (EN): Delta Scuti (delta Sct)(1) stars are opacity-driven pulsators with masses of 1.5-2.5 M(circle dot), their pulsations resulting from the varying ionization of helium. In less massive stars(2) such as the Sun, convection transports mass and energy through the outer 30 per cent of the star and excites a rich spectrum of resonant acoustic modes. Based on the solar example, with no firm theoretical basis, models predict that the convective envelope in delta Sct stars extends only about 1 per cent of the radius(3), but with sufficient energy to excite solar-like oscillations(4,5). This was not observed before the Kepler mission(6), so the presence of a convective envelope in the models has been questioned. Here we report the detection of solar-like oscillations in the delta Sct star HD187547, implying that surface convection operates efficiently in stars about twice as massive as the Sun, as the ad hoc models predicted.
Language: English
Type (Professor's evaluation): Scientific
No. of pages: 4
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