| 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
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.