Issue |
A&A
Volume 388, Number 1, June II 2002
|
|
---|---|---|
Page(s) | 149 - 157 | |
Section | Galactic structure, stellar clusters, and populations | |
DOI | https://doi.org/10.1051/0004-6361:20020447 | |
Published online | 28 May 2002 |
CCD photometry in the Vilnius system in the vicinity of the globular cluster M 56
1
Dip. di Fisica, Università degli Studi di Roma “La Sapienza”, P.le A. Moro 2, 00185 Roma, Italy
2
Vatican Observatory, 00120 Città del Vaticano, Italy
Corresponding author: F. Smriglio, staff@specola.va
Received:
5
July
2000
Accepted:
4
January
2002
CCD observations of field stars in an
area north-east of the globular cluster M 56 were obtained in six
bands of the Vilnius photometric system. The data sets cover a
field of . An outline of the data
pathway from observations to reduction via IRAF is outlined in this text.
Photometry of 366 stars brighter than 18th V magnitude has been
obtained
and the analysis of the observational errors is discussed.
Key words: stars: fundamental parameters / stars: general / galaxy: globular clusters: individual: M 56
© ESO, 2002
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