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A&A 433, L17-L20 (2005)
DOI: 10.1051/0004-6361:200500010
Letter
Exceptional H
emission in the Antennae galaxies:
Pre-starburst shocks from the galaxy collision
M. Haas1, R. Chini1 and U. Klaas2 1 Astronomisches Institut, Ruhr-Universität Bochum (AIRUB), Universitätsstr. 150 / NA7, 44780 Bochum, Germany
e-mail: haas@astro.rub.de
2 Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
(Received 13 December 2004 / Accepted 20 January 2005 )
Abstract
The collision of gas-rich galaxies is believed to produce strong
shocks between their gas clouds which cause the onset of the observed
bursts of extended star formation.
However, the so far observed shock signatures in colliding galaxies
can be explained essentially by winds from already existing massive
stars and supernovae and thus do not give any evidence for an
outstanding pre-starburst phase.
Either pre-starburst gas shocks are too short-lived to be detected
or one has to modify our perception of colliding galaxies.
A dedicated analysis of ISOCAM-CVF mid-infrared spectral maps led us
to the discovery of exceptional
H
v = 0-0 S(3)
= 9.66
m line emission from
the "Antennae" galaxy pair, which is at an early stage of galaxy collision.
Its H
line luminosity, normalized by the far-infrared
luminosity, exceeds that of all
other known galaxies and the strongest H
emission is spatially
displaced from the known starbursts regions. This implies that most of
the excited H
gas in the Antennae must be shocked due to the
collision of the two galaxies. These observations indicate that the
outstanding phase of pre-starburst shocks exists, and that they might
be a key to our understanding of the formation of the first
proto-galaxies.
Key words: galaxies: interacting -- galaxies: ISM -- galaxies: starburst -- galaxies: evolution -- galaxies: individual: Antennae
SIMBAD Objects
© ESO 2005
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