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Astron. Astrophys. 319, 363-363 (1997)

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On the hot ends of the white dwarf spectral sequences: Hot white dwarfs containing helium from the Hamburg-Schmidt survey (Letter)

U. Heber 1, S. Dreizler 1, 2 and H.-J. Hagen 3

1 Dr.-Remeis-Sternwarte, Universität Erlangen-Nürnberg, Sternwartstr. 7, D-96049 Bamberg, Germany
2 Institut für Astronomie und Astrophysik der Universität, D-24098 Kiel, Germany
3 Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany

Astron. Astrophys. 311, L17-L20 (1996)

Due to an object confusion in our observation log file one DAO star is misidentified. The DAO star discussed is HS 2033+0507, not HS 2033+0327 as claimed in the letter. The coordinates of HS 2033+0507 are:


and its apparent magnitude is [FORMULA].

These numbers should replace row 11 of Table 1.

© European Southern Observatory (ESO) 1997

Online publication: July 3, 1998