Issue |
A&A
Volume 423, Number 2, August IV 2004
|
|
---|---|---|
Page(s) | 481 - 493 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20034336 | |
Published online | 06 August 2004 |
The nuclear ring in the unbarred galaxy NGC 278: Result of a minor merger?
1
Centre for Astrophysics Research, University of Hertfordshire, Hatfield, Herts AL10 9AB, UK e-mail: j.knapen@star.herts.ac.uk
2
University of Nottingham, School of Physics and Astronomy, University Park, Nottingham, NG7 2RD, UK
3
Department of Physics and Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3YB, UK
4
Kapteyn Astronomical Institute, University of Groningen, Postbus 800, 9700 AV Groningen, The Netherlands
Received:
17
September
2003
Accepted:
24
April
2004
We present fully sampled high angular resolution two-dimensional
kinematics in the Hα spectral line, optical and near-infrared
imaging, as well as 21 cm atomic hydrogen data of the spiral galaxy
NGC 278. This is a small non-barred galaxy, which has a bright star
forming inner region of about 2 kpc in diameter, reminiscent of nuclear
rings seen mainly in barred galaxies. The Hα kinematics show a
disturbed velocity field, which may be partly the result of spiral
density wave streaming motions. The 21 cm data trace the atomic
hydrogen well outside the optical disk. The is not abundant but
clearly shows disturbed morphology and kinematics. We postulate that
the current structure of NGC 278 is a result of a recent interaction
with a small gas-rich galaxy, which is now dispersed into the outer
disk of NGC 278. Non-axisymmetries set up in the disk by this
minor merger may well be the cause of the intense star formation in the
inner region, which can be interpreted as a rare example of a nuclear
ring in a non-barred galaxy. Rather than being induced by a bar, this
nuclear ring would then be the direct result of an interaction event
in the recent history of the galaxy.
Key words: galaxies: individual: NGC 278 / galaxies: ISM / galaxies: kinematics and dynamics / galaxies: spiral / galaxies: structure
© ESO, 2004
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