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Issue A&A
Volume 439, Number 3, September I 2005
Page(s) 1135 - 1135
Section Stellar structure and evolution
DOI http://dx.doi.org/10.1051/0004-6361:20041458e



A&A 439, 1135-1135 (2005)
DOI: 10.1051/0004-6361:20041458e

Erratum

The old open clusters Berkeley 36, Berkeley 73 and Biurakan 13 (Berkeley 34)

S. Ortolani1, E. Bica2, B. Barbuy3 and M. Zoccali4

1  Università di Padova, Dipartimento di Astronomia, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
    e-mail: ortolani@pd.astro.it
2  Universidade Federal do Rio Grande do Sul, Departamento de Astronomia, CP 15051, Porto Alegre 91501-970, Brazil
    e-mail: bica@if.ufrgs.br
3  Universidade de São Paulo, IAG, Rua do Matão 1226, Cidade Universitária, São Paulo 05508-900, Brazil
    e-mail: barbuy@astro.iag.usp.br
4  Universidad Catolica de Chile, Department of Astronomy & Astrophysics, Casilla 306, Santiago 22, Chile
    e-mail: mzoccali@astro.puc.cl

(A&A, 429, 607-612 (2005), DOI: 1021051/0004-6361:20041458)

Erratum of A&A  429 p. 607


Abstract
The coordinates of Berkeley 73 typed in the paper are wrong. The correct ones are J2000 $\alpha = 06^{\rm h}22^{\rm m}05^{\rm s}$, $\delta = -06^{\circ}18'59''\, (l=215.26^{\circ}$, $b=-9.39^{\circ})$. The coordinates in the Galaxy were revised to X=-13.5 kpc, Y=-3.9 kpc, Z=-1.1 kpc, and the distance from the Galactic center $R_{\rm GC} = 14.1$ kpc. We confirm that the cluster images and colour-magnitude diagrams shown in the paper are indeed from Berkeley 73.


Key words: Galaxy: open clusters and associations: individual: Berkeley 36, Berkeley 73, Biurakan 13 -- HR diagram -- errata, addenda


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