A&A 395, 423-429 (2002)
DOI: 10.1051/0004-6361:20021331
PB 9493-9494 intertacting galaxies: The correlation of IRAS sources with close pairs of PB UVe objects
H. Reboul1 and C. Vanderriest21 UMR 5024, CNRS-Université Montpellier 2, GRAAL, CC 72, 34095 Montpellier Cedex 5, France
2 UMR 8631, CNRS-DAEC, Observatoire de Paris, 92195 Meudon, France
(Received 12 September 2000 / Accepted 22 August 2002 )
Abstract
The cross-correlation of close pairs of UV-excess objects from the
Berger-Fringant catalogue with IRAS sources supplies three cases.
The first two are already known objects. We study in detail the most
interesting (and new) case: PB 9493-9494.
Optical observations in direct imaging and in integral field spectrography
confirm that this system is a pair of strongly interacting galaxies
with starbursts and show the complex structure of an evolved but not merged
encounter. Although such an evolution step is only intermediate, the brightest
nucleus (PB 9494) may be on the verge of becoming an AGN.
We discuss the peculiarities of this system with regard to optical
versus far infrared behaviour, in connection with its special mode of selection.
Key words: galaxies: individual: PB 9494, PB 9493 -- galaxies: interactions -- galaxies: starburst -- ultraviolet: galaxies -- infrared: galaxies
Offprint request: H. Reboul, reboul@graal.univ-montp2.fr
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© ESO 2002
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