| Issue |
A&A
Volume 374, Number 1, July IV 2001
|
|
|---|---|---|
| Page(s) | 264 - 264 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361:20010844 | |
| Published online | 15 July 2001 | |
Erratum Empirical relations for cluster RR Lyrae stars revisited
1
Konkoly Observatory, PO Box 67, 1525 Budapest, Hungary
2
Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory (The National Optical Astronomy Observatory is operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Fundation.) , Casilla 603, Chile e-mail: awalker@noao.edu
Corresponding author: G. Kovács, kovacs@konkoly.hu
A& A, 371, 579-591 (2001), DOI: 10.1051/0004-6361:20010346
Because of an unfortunate mistake, a rough reddening correction from
earlier works was left in the average V magnitudes of the variables of
M 4. Therefore, the reddened distance modulus (
) for this
cluster is incorrectly given in Table 9. The correct value of
is -4.43 instead of -5.69 as given in the
paper. The above mistake does not affect any other parts of the paper,
including the dereddened distance moduli of M 4.
© ESO, 2001
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