223 research outputs found
Kinematics in the Central Kiloparsec of Spiral Galaxies
Results from kinematic observations of the central regions of spiral galaxies
are reviewed, with particular emphasis on starburst and AGN hosts. While
morphological studies lead to important insight, a more complete understanding
of the physical processes that drive the evolution of the central regions can
be achieved with measurements of the kinematics of gas and stars. Here, a
variety of observational techniques at different wavelengths is critically
discussed, and specific areas of interest are highlighted, such as inflow in
barred galaxies and the origin of nuclear spiral arms. A brief discussion of a
number of case studies is presented to illustrate recent progress.Comment: Invited review, to appear in The Central kpc of Starbursts and AGN:
the La Palma Connection, eds. J. H. Knapen, J. E. Beckman, I. Shlosman, and
T. J. Mahoney (ASP: San Francisco), Vol. 249. 18 pages latex, includes 9
postscript figures. Uses newpasp.sty (included
High-resolution UKIRT observations of circumnuclear star formation in M100
We present high-resolution, near-infrared imaging of the circumnuclear region
of the barred spiral galaxy M100 (=NGC 4321), accompanied by near-infrared
spectroscopy. We identify a total of 43 distinct regions in the K-band image,
and determine magnitudes and colours for 41 of them. By comparison with other
near-infrared maps we also derive colour excesses and K-band extinctions for
the knots. Combining the imaging and spectroscopic results, we conclude that
the knots are the result of bursts of star formation within the last 15-25 Myr.
We discuss the implications of these new results for our dynamical and
evolutionary understanding of this galaxy.Comment: 10 pages, 4 figures, uses mn-1.4.sty. Accepted for publication in
Monthly Notices of the Royal Astronomical Societ
Deficiency of `Thin' Stellar Bars in Seyfert Host Galaxies
Using all available major samples of Seyfert galaxies and their corresponding
control samples of closely matched non-active galaxies, we find that the bar
ellipticities (or axial ratios) in Seyfert galaxies are systematically
different from those in non-active galaxies. Overall, there is a deficiency of
bars with large ellipticities (i.e., `fat' or `weak' bars) in Seyferts,
compared to non-active galaxies. Accompanied with a large dispersion due to
small number statistics, this effect is strictly speaking at the `2sigma'
level. To obtain this result, the active galaxy samples of near-infrared
surface photometry were matched to those of normal galaxies in type, host
galaxy ellipticity, absolute magnitude, and, to some extent, in redshift. We
discuss possible theoretical explanations of this phenomenon within the
framework of galactic evolution, and, in particular, of radial gas
redistribution in barred galaxies. Our conclusions provide further evidence
that Seyfert hosts differ systematically from their non-active counterparts on
scales of a few kpc.Comment: Astrophysical Journal Letters, in press. Latex, 2 postscript figure
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