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A&A 383, 472-490 (2002)
DOI: 10.1051/0004-6361:20011757
Detection of a thick disk in the edge-on low surface brightness galaxy ESO 342-G017
I. VLT Photometry in
and
bands
M. J. Neeser1, 2, P. D. Sackett1, G. De Marchi3 and F. Paresce4
1 Kapteyn Astronomical Institute, Postbus 800, 9700 AV Groningen, The Netherlands
2 Universitäts-Sternwarte München, Scheinerstr. 1, 81679 München, Germany
3 European Space Agency, Research and Science Support Department, 3700 San Martin Drive, Baltimore, MD 21218, USA
4 European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany
(Received 5 October 2001 / Accepted 6 December 2001 )
Abstract
We report the detection of a thick disk in the edge-on,
low surface brightness (LSB), late-type spiral , based on
ultra-deep images in the
V and
R bands obtained
with the VLT Test Camera during Science Verification on UT1.
All steps in the reduction procedure are fully described,
which, together with an extensive analysis of systematic and
statistic uncertainties, has resulted in surface brightness
photometry that is reliable for the detection of faint
extended structure to a level of
V = 27.5 and
R = 28.5 . The faint light apparent in these
deep images is well-modeled by a thick exponential disk
with an intrinsic scale height about 2.5 times that of the
thin disk, and a comparable or somewhat larger scale length.
Deprojection including the effects of inclination and
convolution with the PSF allow us to estimate that the
thick disk contributes 20-40% of the total (old) stellar
disk luminosity of .
To our knowledge, this is the first detection of a thick disk in
an LSB galaxy, which are generally thought to be rather unevolved
compared to higher surface brightness galaxies.
Key words: galaxies: spiral, stellar content, structure
Offprint request: M. J. Neeser, neeser@usm.uni-muenchen.de
SIMBAD Objects
© ESO 2002
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