EDP Sciences
Free access
Volume 379, Number 3, December I 2001
Page(s) 845 - 854
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20011371
A&A 379, 845-854 (2001)
DOI: 10.1051/0004-6361:20011371

The merger stage of the ultra-luminous infrared galaxy IRAS 03158+4227

H. Meusinger1, B. Stecklum1, C. Theis2 and J. Brunzendorf1

1  Thüringer Landessternwarte Tautenburg, 07778 Tautenburg, Germany
2  Institut für Theoretische Physik und Astrophysik der Universität Kiel, Olshausenstr. 40, 24098 Kiel, Germany

(Received 12 July 2001 / Accepted 24 September 2001 )

We examine the merger stage of IRAS 03158+4227, one of the most luminous ULIRGs from the IRAS 2 Jy sample. Deep optical images are presented along with high-resolution NIR images and optical low-resolution spectra. IRAS 03158+4227 is confirmed as a component of an equal-luminosity binary galaxy with a nuclei separation of 47 h75-1 kpc. A long lopsided tail emanating from the companion, which harbours an active nucleus, is the most prominent peculiar feature of the binary. The results of numerical simulations permit the interpretation of this structure as a product of the tidal interaction between the two components. If the infrared-activity of IRAS 03158+4227 is also dynamically triggered by this process, this would imply that the ULIRG phenomenon is not restricted to the final stage of a binary merger. Alternatively, the system may be a multiple merger where the partner(s) has/have already coalesced.

Key words: galaxies: interactions -- galaxies: nuclei -- galaxies: starbursts -- infrared: galaxies

Offprint request: H. Meusinger, meus@tls-tautenburg.de

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