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A near Infrared Speckle Imaging Study of T Tauri Stars

Ghez, A. M. and Mccarthy, D. W. and Weinberger, A. J. and Neugebauer, G. and Matthews, K. (1994) A near Infrared Speckle Imaging Study of T Tauri Stars. In: Infrared Astronomy with Arrays: The Next Generation. Astrophysics and Space Science Library. No.190. Springer , Dordrecht, pp. 449-452. ISBN 978-94-010-4466-0. https://resolver.caltech.edu/CaltechAUTHORS:20170227-155358815

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Abstract

The results of a speckle imaging survey of T Tauri stars suggest that most, if not all, young low mass stars have companions. Repeated observations of these young binary stars have revealed orbital motion in the closest pairs (≤ 0.″3), proving that these systems are indeed gravitationally bound and providing the basis for mass estimates in the upcoming years. These mass estimates are necessary to distinguish between the various binary star formation mechanisms that have been proposed to date.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1007/978-94-011-1070-9_135DOIArticle
ORCID:
AuthorORCID
Ghez, A. M.0000-0003-3230-5055
Weinberger, A. J.0000-0001-6654-7859
Additional Information:© 1994 Springer Science+Business Media Dordrecht.
Subject Keywords:T Tauri Stars – Binary Stars – Speckle Imaging
Series Name:Astrophysics and Space Science Library
Issue or Number:190
Record Number:CaltechAUTHORS:20170227-155358815
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170227-155358815
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:74564
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:28 Feb 2017 00:04
Last Modified:06 Mar 2020 15:49

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