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Precision masses of the low-mass binary system GJ 623

Martinache, Frantz and Lloyd, James P. and Ireland, Michael J. and Yamada, Ryan S. and Tuthill, Peter G. (2007) Precision masses of the low-mass binary system GJ 623. Astrophysical Journal, 661 (1). pp. 496-501. ISSN 0004-637X. doi:10.1086/513868. https://resolver.caltech.edu/CaltechAUTHORS:MARapj07

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Abstract

We have used aperture masking interferometry and adaptive optics (AO) at the Palomar 200 inch telescope to obtain precise mass measurements of the binary M dwarf GJ 623. AO observations spread over 3 yr combined with a decade of radial velocity measurements constrain all orbital parameters of the GJ 623 binary system accurately enough to critically challenge the models. The dynamical masses measured are m(1) = 0.371 ± 0.015 M☉ (4%) and m(2) = 0.115 ± 0.0023 M☉ (2%) for the primary and the secondary, respectively. Models are not consistent with color and mass, requiring very low metallicities.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/513868DOIArticle
ORCID:
AuthorORCID
Martinache, Frantz0000-0003-1180-4138
Ireland, Michael J.0000-0002-6194-043X
Additional Information:© 2007 American Astronomical Society. Received 2006 December 4; accepted 2007 February 7. We thank the staff and telescope operators of Palomar Observatory and Keck Observatory for their support. F.M. thanks Terry Herter for his help. This work is partially funded by the National Science Foundation under grants AST 03-35695 and AST 05-06588. This publication makes use of the Simbad database, operated at CDS, Strasbourg, France and the data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. We wish to extend special thanks to those of Hawaiian ancestry on whose sacred mountain we are privileged to be guests. Without their generous hospitality, the observations presented herein would not have been possible.
Funders:
Funding AgencyGrant Number
NSFAST 03-35695
NSFAST 05-06588
NASAUNSPECIFIED
Subject Keywords:binaries: general; stars: luminosity function, mass function; techniques: interferometric
Issue or Number:1
DOI:10.1086/513868
Record Number:CaltechAUTHORS:MARapj07
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:MARapj07
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:12065
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:22 Oct 2008 16:23
Last Modified:08 Nov 2021 22:25

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