The red-giant CoRoT target HR 7349

F Carrier; T Morel; A Miglio; J Montalban; M Auvergne; A Baglin; F Baudin; Saskia Hekker

doi:10.1007/s10509-009-0171-y

The red-giant CoRoT target HR 7349

F Carrier, T Morel, A Miglio, J Montalban, M Auvergne, A Baglin, F Baudin, Saskia Hekker

Physics and Astronomy

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2 Citations (Scopus)

Abstract

HR 7349 is a bright [V = 5.8] red giant observed by CoRoT in the seismofield of the first long run. The outstanding CoRoT light curve allowed the detection of several solar-like oscillation modes (both radial and non-radial). On top of these seismic constraints, our observational knowledge on HR 7349 benefits as well from a precise parallax and detailed spectroscopic constraints. We present all the observational constraints that are available for the theoretical modelling of this most promising target.

Original language	English
Journal	Astrophysics and Space Science
DOIs	https://doi.org/10.1007/s10509-009-0171-y
Publication status	Published - 20 Oct 2009

Keywords

Stars: variables
Stars: oscillations
Stars: interiors

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10.1007/s10509-009-0171-y

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title = "The red-giant CoRoT target HR 7349",

abstract = "HR 7349 is a bright [V = 5.8] red giant observed by CoRoT in the seismofield of the first long run. The outstanding CoRoT light curve allowed the detection of several solar-like oscillation modes (both radial and non-radial). On top of these seismic constraints, our observational knowledge on HR 7349 benefits as well from a precise parallax and detailed spectroscopic constraints. We present all the observational constraints that are available for the theoretical modelling of this most promising target.",

keywords = "Stars: variables, Stars: oscillations, Stars: interiors",

author = "F Carrier and T Morel and A Miglio and J Montalban and M Auvergne and A Baglin and F Baudin and Saskia Hekker",

year = "2009",

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doi = "10.1007/s10509-009-0171-y",

language = "English",

journal = "Astrophysics and Space Science",

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T1 - The red-giant CoRoT target HR 7349

AU - Carrier, F

AU - Morel, T

AU - Miglio, A

AU - Montalban, J

AU - Auvergne, M

AU - Baglin, A

AU - Baudin, F

AU - Hekker, Saskia

PY - 2009/10/20

Y1 - 2009/10/20

N2 - HR 7349 is a bright [V = 5.8] red giant observed by CoRoT in the seismofield of the first long run. The outstanding CoRoT light curve allowed the detection of several solar-like oscillation modes (both radial and non-radial). On top of these seismic constraints, our observational knowledge on HR 7349 benefits as well from a precise parallax and detailed spectroscopic constraints. We present all the observational constraints that are available for the theoretical modelling of this most promising target.

AB - HR 7349 is a bright [V = 5.8] red giant observed by CoRoT in the seismofield of the first long run. The outstanding CoRoT light curve allowed the detection of several solar-like oscillation modes (both radial and non-radial). On top of these seismic constraints, our observational knowledge on HR 7349 benefits as well from a precise parallax and detailed spectroscopic constraints. We present all the observational constraints that are available for the theoretical modelling of this most promising target.

KW - Stars: variables

KW - Stars: oscillations

KW - Stars: interiors

U2 - 10.1007/s10509-009-0171-y

DO - 10.1007/s10509-009-0171-y

M3 - Article

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

ER -

The red-giant CoRoT target HR 7349

Abstract

Keywords

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