HR 7322: A benchmark of stellar evolution

Research output: Contribution to conferencePosterResearch

HR 7322 is a bright F6 subgiant star in the Kepler field, which has been used as a comparison star in spectroscopy and photometry. HR 7322 has not been the subject of detailed studies before, but using interferometry and asteroseismology we have made an in-depth analysis of HR 7322. The derived stellar parameters are used in order to find the constraints needed for stellar modelling and thus to test -- and improve -- our current models of stellar structure and evolution.
Original languageEnglish
Publication yearJul 2017
Publication statusPublished - Jul 2017
EventThe TASC3/KASC10 workshop: TESSting Stellar Astrophysics - University of Birmingham, Birmingham, United Kingdom
Duration: 16 Jul 201721 Jul 2017


WorkshopThe TASC3/KASC10 workshop
LocationUniversity of Birmingham
CountryUnited Kingdom
Internet address

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ID: 121026342