Belt(s) of debris resolved around the Sco-Cen star HIP 67497⋆⋆⋆

Author： Bonnefoy M.   Milli J.   Ménard F.   Vigan A.   Lagrange A.-M.   Delorme P.   Boccaletti A.   Lazzoni C.   Galicher R.   Desidera S.   Chauvin G.   Augereau J. C.   Mouillet D.   Pinte C.   van der Plas G.   Gratton R.   Beust H.   Beuzit J. L.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|597|issue|L7-L7

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.597, Iss.issue, 2017-01, pp. : L7-L7

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

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Abstract

Aims. In 2015, we initiated a survey of Scorpius-Centaurus A-F stars that are predicted to host warm-inner and cold-outer belts of debris similar to the case of the system HR 8799. The survey aims to resolve the disks and detect planets responsible for the disk morphology. In this paper, we study the F-type star HIP 67497 and present a first-order modelization of the disk in order to derive its main properties.

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