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Multiplicity Study of Exoplanet Host Stars: the HD 3651 AB System

Published online by Cambridge University Press:  09 August 2007

M. Mugrauer ,
A. Seifahrt ,
R. Neuhäuser ,
T. Mazeh  and
T. Schmidt
M. Mugrauer
Affiliation:
Astrophysikalisches Institut, Universität Jena, Schillergäßchen 2-3, 07745 Jena, Germany
A. Seifahrt
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany
R. Neuhäuser
Affiliation:
Astrophysikalisches Institut, Universität Jena, Schillergäßchen 2-3, 07745 Jena, Germany
T. Mazeh
Affiliation:
Tel Aviv University, Tel Aviv 69978, Israel
T. Schmidt
Affiliation:
Astrophysikalisches Institut, Universität Jena, Schillergäßchen 2-3, 07745 Jena, Germany
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Abstract

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We report on new results of our multiplicity study and present our follow-up observations of the recently detected faint companion HD 3651 B, the first directly–imaged T dwarf companion of an exoplanet host star.

Keywords

(stars:) binaries: visualstars: low-massbrown dwarfs
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S240: Binary Stars as Critical Tools & Tests in Contemporary Astrophysics , August 2006 , pp. 638 - 640
Copyright
Copyright © International Astronomical Union 2007

References

Burgasser, A.J., et al. , 2000, ApJL, 531, L57 Google Scholar
Burgasser, A.J., et al. 2002, APJ, 564, 421 CrossRefGoogle Scholar
Burgasser, A.J., 2006, arXiv:astro-ph/0609556Google Scholar
Butler, R.P., Tinney, C.G., Marcy, G.W., Jones, H.R.A., Penny, A.J. 2001, ApJ, 555, 410 Google Scholar
Holman, M. J., & Wiegert, P. A.: 1999, AJ, 117, 621 Google Scholar
Knapp, G.R., et al. 2004, AJ, 127, 3553 Google Scholar
Lagrange, A.-M., Beust, H., Udry, S., Chauvin, G., & Mayor, M. 2006, arXiv:astro-ph/0606167Google Scholar
Luhman, K.L., et al. 2006, arXiv:astro-ph/0609464Google Scholar
Mugrauer, M., Neuhäuser, R., Mazeh, T., Guenther, E., & Fernández, M. 2004a, AN, 325, 718 Google Scholar
Mugrauer, M., Neuhäuser, R., Mazeh, T., Alves, J., & Guenther, E. 2004b, A&A, 425, 249 Google Scholar
Mugrauer, M., Neuhäuser, R., Seifahrt, A., Mazeh, T., & Guenther, E. 2005, A&A, 440, 1051 Google Scholar
Mugrauer, M., & Neuhäuser, R. 2005, MNRAS, 361, L15 Google Scholar
Mugrauer, M., Neuhäuser, R., Mazeh, T., & Guenther, E. 2006a, tafp.conf, 314Google Scholar
Mugrauer, M., Neuhäuser, R., Mazeh, T., Guenther, E., Fernández, M. 2006b, AN, 327, 321 Google Scholar
Mugrauer, M., Seifahrt, A., Neuhaeuser, R., & Mazeh, T. 2006c, arXiv:astro-ph/0608484Google Scholar
Pichardo, B., Sparke, L.S., & Aguilar, L.A. 2005, MNRAS, 359, 521 Google Scholar
Skrutskie, M.F., et al. 2006, AJ, 131, 1163 CrossRefGoogle Scholar
Queloz, D., et al. 2000, A&A, 354, 99 Google Scholar
Weidemann, V. 2000, A&A, 363, 647 Google Scholar
Worley, C.E., & Douglass, G.G. 1997, AAPS, 125, 523 Google Scholar