Discovery of an Extended Debris Disk around the F2 V Star HD 15745

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Published 2007 November 26 © 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Paul Kalas et al 2007 ApJ 671 L161 DOI 10.1086/525252

1538-4357/671/2/L161

Abstract

Using the Advanced Camera for Surveys aboard the Hubble Space Telescope, we have discovered dust-scattered light from the debris disk surrounding the F2 V star HD 15745. The circumstellar disk is detected between 2.0'' and 7.5'' radius, corresponding to 128-480 AU radius. The circumstellar disk morphology is asymmetric about the star, resembling a fan, and consistent with forward scattering grains in an optically thin disk with an inclination of ~67° to our line of sight. The spectral energy distribution and scattered light morphology can be approximated with a model disk composed of silicate grains between 60 and 450 AU radius, with a total dust mass of 10−7 M (0.03 M), representing a narrow grain size distribution (1-10 μm). Galactic space motions are similar to the Castor moving group, with an age of ~108 yr, although future work is required to determine the age of HD 15745 using other indicators.

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10.1086/525252