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Interferometry to Determine Stellar Shapes: Application to Achernar

Abstract : The shape of stellar photospheres can depart significantly from the spherical geometry, due e.g. to fast rotation. In this chapter, I focus on the application of long-baseline interferometry to the determination of the photospheric shape of fast rotating stars. I present the example of the VLT Interferometer observations of the nearby Be star Achernar (α Eri), using the VINCI (two telescopes) and PIONIER (four telescopes) beam combiners. I present the adjustment of a simplified model of the light distribution of Achernar to the measured interferometric visibilities and closure phases . This example application is based on the LITpro software from the JMMC.
Keywords : Physics
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Contributor : Nathalie POTHIER Connect in order to contact the contributor
Submitted on : Thursday, April 7, 2022 - 3:07:01 PM
Last modification on : Saturday, April 9, 2022 - 3:39:03 AM



Pierre Kervella. Interferometry to Determine Stellar Shapes: Application to Achernar. Cartography of the Sun and the Stars, pp.127-135, 2016, ⟨10.1007/978-3-319-24151-7_6⟩. ⟨insu-03634271⟩



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