arXiv · astro-ph/9812187
A Candidate Substellar Companion to CoD -33 7795 (TWA 5)
Abstract
We present the discovery of a candidate substellar object in a survey of young stars in the solar vicinity using the sensitivity and spatial resolution afforded by the NICMOS coronagraph on the Hubble Space Telescope. The H=12.1 mag object was discovered approximately 2 arcsec from the TW Hydrae Association member CoD -33 7795 (TWA 5), and the photometry implies a spectral type M8-M8.5, with a temperature of approximately 2600K. We estimate that the probability of a chance alignment with a background objectof this nature is < 2 X 10^(-5), and therefore postulate the object (TWA 5B) is physically associated at a projected separation of 100 AU. Given the likely youth of the primary (~ 10 Myr), current brown dwarf cooling models predict a mass of approximately 20 Jupiter masses for TWA 5B.
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P. J. Lowrance, C. McCarthy, E. E. Becklin, B. Zuckerman, G. Schneider, R. A. Webb, D. C. Hines, J. D. Kirkpatrick, D. W. Koerner, F. Low, R. Meier, M. Rieke, B. A. Smith, R. J. Terrile, R. I. Thompson. 1998-12-09. A Candidate Substellar Companion to CoD -33 7795 (TWA 5). https://doi.org/10.1086/311858
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