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Astron. Astrophys. 364, 926 (2000)

Table of Contents

Erratum

Hot HB stars in globular custers - Physical parameters and consequences for theory

V. Radiative levitation versus helium mixing

S. Moehler 1, A.V. Sweigart 2, W.B. Landsman 3 and U. Heber 1

1 Dr. Remeis-Sternwarte, Astronomisches Institut der Universität Erlangen-Nürnberg, Sternwartstrasse 7, 96049 Bamberg, Germany (moehler@sternwarte.uni-erlangen.de; heber@sternwarte.uni-erlangen.de)
2 NASA Goddard Space Flight Center, Code 681, Greenbelt, MD 20771, USA (sweigart@bach.gsfc.nasa.gov)
3 Raytheon ITSS, NASA Goddard Space Flight Center, Code 681, Greenbelt, MD 20771, USA (landsman@mpb.gsfc.nasa.gov)

Astron. Astrophys. 360, 120--132 (2000)

As the result of an unfortunate error during printing of the article the following Note added in proof has not been inserted as indicated by the authors.

Note added in proof. With respect to the rotational velocities of blue HB stars in globular clusters Soker & Harpaz (2000, MNRAS 317, 861) recently suggested that a spin-up of red giants by planets, brown dwarfs, or low-mass stars and the resulting increases in loss of mass and angular momentum could explain the observations.

Table of Contents

© European Southern Observatory (ESO) 2000

Online publication: January 29, 2001
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