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 | ||||||
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| 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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