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The large scale magnetic field of the G0 dwarf HD 206860 (HN Peg)

Published online by Cambridge University Press:  07 August 2014

Sudeshna Boro Saikia ,
Sandra V. Jeffers ,
Pascal Petit ,
Stephen Marsden ,
Julien Morin ,
Ansgar Reiners  and
the Bcool project
Sudeshna Boro Saikia
Affiliation:
Institut für Astrophysik, Universität Göttingen Friedrich Hund Platz 1, 37077, GöttingenGermany email: [email protected], [email protected], [email protected]
Sandra V. Jeffers
Affiliation:
Institut für Astrophysik, Universität Göttingen Friedrich Hund Platz 1, 37077, GöttingenGermany email: [email protected], [email protected], [email protected]
Pascal Petit
Affiliation:
CNRS, Institut de Recherche en Astrophysique et Planétologie 14 Avenue Edouard Belin, F-31400 Toulouse, France email: [email protected]
Stephen Marsden
Affiliation:
Faculty of Sciences, University of Southern Queensland Toowoomba 4350, Australia email: [email protected]
Julien Morin
Affiliation:
Institut für Astrophysik, Universität Göttingen Friedrich Hund Platz 1, 37077, GöttingenGermany email: [email protected], [email protected], [email protected]
Ansgar Reiners
Affiliation:
Institut für Astrophysik, Universität Göttingen Friedrich Hund Platz 1, 37077, GöttingenGermany email: [email protected], [email protected], [email protected]
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Abstract

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HD 206860 is a young planet (HN Peg b) hosting star of spectral type G0V and it has a potential debris disk around it. In this work we measure the longitudinal magnetic field of HD 206860 using spectropolarimetric data and we measure the chromospheric activity using Ca II H&K, H-alpha and Ca II infrared triplet lines.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S302: Magnetic Fields throughout Stellar Evolution , August 2013 , pp. 146 - 147
Copyright
Copyright © International Astronomical Union 2014 

References

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