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A&A 440, 783-789 (2005)
DOI: 10.1051/0004-6361:20042012
A survey for OB associations in the Sculptor Group spiral galaxy NGC 7793
G. Pietrzynski1, 2, K. Ulaczyk2, W. Gieren1, F. Bresolin3 and R. P. Kudritzki31 Universidad de Concepción, Departamento de Fisica, Casilla 160-C, Concepción, Chile
e-mail: pietrzyn@hubble.cfm.udec.cl; wgieren@astro-udec.cl
2 Warsaw University Observatory, AL. Ujazdowskie 4, 00-478 Warsaw, Poland
e-mail: kulaczyk@astrouw.edu.pl
3 Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, Hawaii, USA
e-mail: [bresolin; kud]@ifa.hawaii.edu
(Received 15 September 2004 / Accepted 13 April 2005)
Abstract
We report on the results from application of an objective algorithm (PLC)
to find OB associations, to B and V images of the Sculptor spiral galaxy NGC 7793, which
were obtained with the ESO VLT and FORS instrument and basically cover the entire spatial extent of the galaxy.
We detected 148 associations. Statistical tests show that less than 6 of these detections are caused by
randomly concentrated blue stars. In the size distribution, a sharp peak is observed at a
value of about 35 microradians, which corresponds to a linear diameter of 135 pc, assuming a distance
of 3.91 Mpc to the galaxy. We also find 25 much larger objects. A second application of the PLC technique shows
that 20 of them are stellar complexes consisting of multiple sub-associations with typical sizes on the order
of 130 pc.
A comparison of the size distribution of the detected OB associations in NGC 7793 with observed
distributions in other galaxies suggests that the conditions in two
Sculptor Group galaxies (NGC 300 and NGC 7793) favour the formation of large associations.
We provide a catalog giving coordinates and physical parameters
for all the associations and stellar complexes we have found in our survey.
Key words: Galaxy: open clusters and associations: individual: galaxy: NGC 7793
SIMBAD Objects
© ESO 2005
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