Astron. Astrophys. 358, 1077-1089 (2000)
Strömgren photometry towards the region of the Cometary Globules CG 30/31/38 *
A.S. Nielsen,
H. Jonch-Sorensen and
J. Knude
Niels Bohr Institute for Astronomy, Geophysics and Physics, Juliane Maries Vej 32, 2100 Kobenhavn O, Denmark (alan@astro.ku.dk)
Received 24 March 2000 / Accepted 26 April 2000
Abstract
With the Danish 1.54 m telescope at La Silla, Chile, we have
obtained deep ( ) CCD frames in the
Strömgren system towards
the region of the cometary globules CG 30/31/38. Also, a nearby
reference field, with a minor amount of visible molecular material,
has been observed in order to estimate the expected normal
foreground reddening in this direction of the Galaxy. We have obtained
complete information for 698 and 526
stars in these two regions, respectively, allowing a determination of
individual stellar extinctions and distances for the A- to G-type star
subsample meeting the criteria in the calibrations. A lower envelope
in the distance-reddening diagram ( )
indicates that the minimum total absorption through half the Galactic
disk along the line of sight is in
this direction. The distance to the CG 30/31/38 complex is not
directly derived from the -diagram but
two faint foreground M-dwarfs are identified, and based on the
obtained photometry a lower distance
limit of 215 40 pc is derived.
We also report the discovery of a galaxy seen in V and
I-band exposures in spite of the high extinction, located at
the very low galactic latitude of
.
Key words: ISM:
clouds
ISM: dust, extinction
* Based on observations ESO, La Silla
SIMBAD Objects
Contents
© European Southern Observatory (ESO) 2000
Online publication: June 20, 2000
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