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A&A 378, L10-L13 (2001)
DOI: 10.1051/0004-6361:20011205
A close look into an intermediate redshift galaxy using STIS
D. F. de Mello1 and A. Pasquali21 Onsala Space Observatory, Chalmers University of Technology, 43992 Onsala, Sweden
2 ESO/ST-ECF, Karl-Schwarzschild-Strasse 2, 85748 Garching bei Muenchen, Germany
e-mail: apasqual@eso.org
(Received 6 June 2001 / Accepted 26 August 2001 )
Abstract
We present a detailed view of a galaxy at z=0.4 which is part of a
large database of intermediate redshifts using high resolution images. We used the
STIS parallel images and spectra to identify the object and obtain
the redshift. The high resolution STIS image (0.05'') enabled us to analyse the
internal structures of this galaxy. A bar along the major axis and hot-spots of
star formation separated by 0.37'' (1.6 kpc) are found along the inner region
of the galaxy. The analysis of the morphology of faint galaxies like this one is an
important step towards estimating the epoch of formation of the Hubble classification
sequence.
Key words: faint galaxies -- barred galaxies -- mergers -- galaxy evolution
Offprint request: D. F. de Mello, duilia@oso.chalmers.se
SIMBAD Objects
© ESO 2001
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