2009A&A...506.1541A


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.04CEST21:53:28

2009A&A...506.1541A - Astronomy and Astrophysics, volume 506, 1541-1562 (2009/11-2)

PMAS optical integral field spectroscopy of luminous infrared galaxies. I. The atlas.

ALONSO-HERRERO A., GARCIA-MARIN M., MONREAL-IBERO A., COLINA L., ARRIBAS S., ALFONSO-GARZON J. and LABIANO A.

Abstract (from CDS):

Luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) are key cosmological classes since they account for most of the co-moving star formation rate density at z∼1-2. It is then important to have detailed studies of local samples of their counterparts for understanding the internal and dynamical processes taking place at high-z. To characterize the two-dimensional morphological, excitation and kinematic properties of LIRGs and ULIRGs we are carrying out an optical integral field spectroscopy (IFS) survey of local (z<0.26) samples. In this paper we present optical (3800-7200Å) IFS with the Potsdam multi-aperture spectrophotometer (PMAS) of the northern hemisphere portion of a volume-limited (2750-5200km/s) sample of 11 LIRGs. The PMAS IFS observations typically cover the central ∼5kpc and are complemented with our own existing HST/NICMOS images. For most LIRGs in our sample, the peaks of the continuum and gas (e.g., Hα, [NII]λ6584) emissions coincide, unlike what is observed in local, strongly interacting ULIRGs. The only exceptions are galaxies with circumnuclear rings of star formation where the most luminous Hα emitting regions are found in the rings rather than in the nuclei of the galaxies, and the displacements are well understood in terms of differences in the stellar populations. A large fraction of the nuclei of these LIRGs are classified as LINER and intermediate LINER/HII, or composite objects, which is a combination of starformation and AGN activity. The excitation conditions of the integrated emission depend on the relative contributions of HII regions and the diffuse emission to the line emission over the PMAS FoV. Galaxies dominated by high surface-brightness HII regions show integrated HII-like excitation. A few galaxies show slightly larger integrated [NII]λ6584/Hα and [SII]λ6717,6731/Hα line ratios than the nuclear ones, probably because of more contribution from the diffuse emission. The Hα velocity fields over the central few kpc are generally consistent, at least to first order, with rotational motions. The velocity fields of most LIRGs are similar to those of disk galaxies, in contrast to the highly perturbed fields of most local, strongly interacting ULIRGs. The peak of the Hα velocity dispersion coincides with the position of the nucleus and is likely to be tracing mass. All these results are similar to the properties of z∼1 LIRGs, and they highlight the importance of detailed studies of flux-limited samples of local LIRGs.

Abstract Copyright:

Journal keyword(s): Galaxy: evolution - Galaxy: nucleus - galaxies: Seyfert - galaxies: active - infrared: galaxies

Simbad objects: 16

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Number of rows : 16

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 NGC 23 G 00 09 53.411 +25 55 25.46   12.5       ~ 284 3
2 MCG+12-02-001 G 00 54 03.943 +73 05 05.23   16       ~ 88 1
3 UGC 1845 GiG 02 24 07.9832706371 +47 58 10.743777802   15.7       ~ 72 1
4 NGC 2388 GiG 07 28 53.4530354679 +33 49 08.550019911   14.7       ~ 117 2
5 MCG+02-20-003 GiG 07 35 43.416 +11 42 35.29   15.0       ~ 58 0
6 NGC 3690 IG 11 28 31.326 +58 33 41.80   13.19 12.86     ~ 883 4
7 IC 860 LIN 13 15 03.51 +24 37 07.8   14.8       ~ 178 0
8 NGC 5939 GiG 15 24 45.9988477795 +68 43 50.275288474   13.7       ~ 32 0
9 NGC 5936 H2G 15 30 00.846 +12 59 21.55   13.0       ~ 149 1
10 NGC 6701 G 18 43 12.429 +60 39 12.13   12.9       ~ 116 1
11 NGC 7469 Sy1 23 03 15.674 +08 52 25.28 12.60 13.00 12.34     ~ 1885 3
12 NGC 7591 SyG 23 18 16.2683208567 +06 35 09.111064142   13.8       ~ 222 0
13 NGC 7770 GiG 23 51 22.610 +20 05 48.56   14.5       ~ 93 1
14 NGC 7771 GiG 23 51 24.880 +20 06 42.57 13.42 13.08 12.25     ~ 313 4
15 NGC 7771E ~ 23 51 24.88 +20 06 42.6           ~ 2 0
16 NGC 7771W ~ 23 51 24.88 +20 06 42.6           ~ 2 0

    Equat.    Gal    SGal    Ecl

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2020.07.04-21:53:28

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