UBV photometry of galactic foreground and LMC member stars^*,**

II. Galactic foreground stars (supplement)

¹ Astronomisches Institut der Ruhr-Universität, D–44780 Bochum, Germany
² Optikzentrum NRW, Universitätsstraße 142, D–44799 Bochum, Germany
³ Dep. Astrofisica, Pontifica Universidad Catolica de Chile, Casilla 104, Santiago 22, Chile
⁴ Garglasweg 39, CH–7220 Schiers, Switzerland

Send offprint request to: H.-G. Grothues

Received: 2 February 1996
Accepted: 26 March 1996

Abstract

In addition to the list of UBV photometries of 955 galactic foreground stars in the direction to the Large Magellanic Cloud published by Gochermann et al. (1993a), a supplement of 545 stars is presented, which have been measured with the same photometric accuracy. Moreover, less reliable photometries of 379 further foreground stars are listed in a separate table. The homogeneous data base of more than high accuracy photometries represented by these stars has been used to construct a reddening distribution map of the galactic foreground towards the LMC by Oestreicher et al. (1995).