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The Presence of the Wielen Dip in the Disk Stellar Luminosity Function

Published online by Cambridge University Press:  25 April 2016

Sang-Gak Lee
Sang-Gak Lee*
Affiliation:
Department of Astronomy, Seoul National University, Republic of Korea
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Abstract

The disk stellar luminosity function has been redetermined by the mean absolute magnitude method, utilising the proper motion data of the LHS Catalog. The derived luminosity function shows a slightly deeper dip than that found by Wielen (1983) in the same magnitude range.

Type
Invited
Information
Publications of the Astronomical Society of Australia , Volume 9 , Issue 2 , 1991 , pp. 209 - 211
Copyright
Copyright © Astronomical Society of Australia 1991

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