2008AJ....135.1207M


Query : 2008AJ....135.1207M

2008AJ....135.1207M - Astron. J., 135, 1207-1224 (2008/April-0)

Triggered or self-regulated star formation within intermediate redshift luminous infrared galaxies. I. Morphologies and spectral energy distributions.

MELBOURNE J., AMMONS M., WRIGHT S.A., METEVIER A., STEINBRING E., MAX C., KOO D.C., LARKIN J.E. and BARCZYS M.

Abstract (from CDS):

As part of the Center for Adaptive Optics (AO) Treasury Survey (CATS) we imaged a set of 15 intermediate redshift (z ∼ 0.8) luminous infrared (IR) galaxies (LIRGs) with the Keck Laser Guide Star (LGS) AO facility. These galaxies were selected from the Great Observatories Origins Deep Survey (GOODS) southern field, allowing us to combine the high spatial resolution Hubble Space Telescope optical (B, V, i, and z-bands) images with our near-infrared (K'-band) images to study the LIRG morphologies and spatially resolved spectral energy distributions (SEDs). Two thirds of the LIRGs are disk galaxies, with only one third showing some evidence for interactions, minor, or major mergers. In contrast with local LIRG disks (which are primarily barred systems), only 10% of the LIRG disks in our sample contain a prominent bar. While the optical bands tend to show a significant point-like substructure, indicating distributed star formation, the AO K-band images tend to be smooth. They lack point-like structures to a K ∼ 23.5 limit. This places an upper bound on the number of red super giants per blue knot at less than 4000. The SEDs of the LIRGs are consistent with distributed dusty star formation, as exhibited by optical to IR colors redder than allowed by old stellar populations alone. This effect is most pronounced in the galaxy cores, possibly indicating central star formation. We also observed a set of 11 intermediate redshift comparison galaxies, selected to be non-ellipticals with apparent K-band magnitudes comparable to the LIRGs. The "normal" (non-LIRG) systems tended to have lower optical luminosity, lower stellar mass, and more irregular morphology than the LIRGs. Half of the "normal" galaxies have SEDs consistent with intermediate aged stellar populations and minimal dust. The other half show evidence for some dusty star formation, usually concentrated in their cores. Our work suggests that the LIRG disk galaxies are similar to large disk systems today, undergoing self-regulated star formation, only at 10-20 times higher rates.

Abstract Copyright: ∼

Journal keyword(s): galaxies: spiral - galaxies: starburst - galaxies: stellar content - infrared: galaxies - instrumentation: adaptive optics

Nomenclature: Figs, Table 1: [MAW2008] LIRG NN (Nos 1-15), [MAW2008] COMPGAL NN (Nos 1-11).

Simbad objects: 26

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Number of rows : 26
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 ACS-GC 90043490 Sy2 03 32 07.98 -27 42 39.9   23.6922 23.2064 22.3383 21.8034 ~ 51 0
2 GEMS J033208.45-274243.3 G 03 32 08.433 -27 42 43.44   23.1238   22.841 21.7672 ~ 14 0
3 GEMS J033209.41-274235.9 AGN 03 32 09.398 -27 42 36.12   23.077 24.1581 21.803 22.1912 ~ 33 0
4 GEMS J033212.82-274201.5 G 03 32 12.803 -27 42 01.53   22.9887 22.77 22.391 20.868 ~ 21 0
5 GOODS-MUSIC 16311 EmG 03 32 13.062 -27 42 04.81   22.6498 21.9040 21.330 21.2708 ~ 22 0
6 ACS-GC 90045613 Sy2 03 32 13.257 -27 42 40.65   21.6424 20.820 20.164 19.8240 ~ 87 0
7 GEMS J033213.47-274149.7 G 03 32 13.462 -27 41 49.86   23.1779   22.535 21.878 ~ 10 0
8 ACS-GC 90045746 Sy2 03 32 13.8495 -27 42 49.018   23.1221 22.348 21.8155 21.2325 ~ 66 0
9 GEMS J033230.93-274058.4 G 03 32 30.929 -27 40 58.38   22.8690   22.878 21.8911 ~ 15 0
10 GOODS-MUSIC 17706 EmG 03 32 31.042 -27 40 50.18   23.327 24.0126 23.0426 22.5111 ~ 23 0
11 GEMS J033231.48-274118.1 G 03 32 31.480 -27 41 18.14   22.113 22.373 22.664 21.4663 ~ 14 0
12 GOODS J033232.46-274056.6 EmG 03 32 32.461 -27 40 56.57   23.8767     23.1617 ~ 13 0
13 GEMS J033232.90-274123.9 G 03 32 32.897 -27 41 23.90   23.731 23.88 25.121 22.7522 ~ 17 0
14 GEMS J033232.98-274117.1 AGN 03 32 32.984 -27 41 17.06   24.178   22.660 21.7520 ~ 36 0
15 GEMS J033236.16-273955.7 G 03 32 36.166 -27 39 55.66   22.7553 22.237 21.937 21.5981 ~ 9 0
16 GEMS J033236.68-273954.6 G 03 32 36.682 -27 39 54.58   23.0034 22.4207 21.769 21.7467 ~ 17 0
17 ACS-GC 90043401 Sy1 03 32 38.1232741056 -27 39 45.158278032 20.89 20.9342 20.511 20.4095 20.6297 ~ 69 0
18 GNS 4920 G 03 32 52.33706 -27 50 51.9079   22.657   24.265 22.0055 ~ 12 0
19 GEMS J033252.87-275114.7 G 03 32 52.87661 -27 51 14.7805   22.670   23.337 21.8385 ~ 21 0
20 ACS-GC 90040278 Sy1 03 32 52.89 -27 51 19.8   22.837   23.541 22.3247 ~ 56 0
21 GNS 4948 rG 03 32 53.0175 -27 51 04.789   23.849 24.391 23.877 23.0460 ~ 16 0
22 GNS 4918 G 03 32 53.44277 -27 50 51.3064   21.534 21.663 21.289 21.2625 ~ 11 0
23 GEMS J033255.00-275051.5 G 03 32 55.00769 -27 50 51.6844   22.782   23.213 22.0657 ~ 15 0
24 GOODS J033255.68-275345.8 G 03 32 55.67467 -27 53 45.6418   24.185   25.71 23.2268 ~ 11 0
25 GEMS J033255.87-275328.0 EmG 03 32 55.87913 -27 53 28.0352   22.702   23.328 21.9760 ~ 20 0
26 COMBO J0332559-275356 G 03 32 55.9353 -27 53 56.961   22.5040 22.2299 22.112 21.0804 ~ 15 0

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