2021A&A...649A.137P


Query : 2021A&A...649A.137P

2021A&A...649A.137P - Astronomy and Astrophysics, volume 649A137-137 (2021/5-1)

The physical properties of local (U)LIRGs: A comparison with nearby early- and late-type galaxies.

PASPALIARIS E.-D., XILOURIS E.M., NERSESIAN A., MASOURA V.A., PLIONIS M., GEORGANTOPOULOS I., BIANCHI S., KATSIOLI S. and MOUNTRICHAS G.

Abstract (from CDS):


Aims. In order to pinpoint the place of the (ultra-) luminous infrared galaxies ((U)LIRGs) in the local Universe, we examine the properties of a sample of 67 such nearby systems and compare them with those of 268 early- and 542 late-type, well studied, galaxies from the DustPedia database.
Methods. We made use of multi-wavelength photometric data (from the ultra-violet to the sub-millimetre), culled from the literature, and the CIGALE spectral energy distribution fitting code to extract the physical parameters of each system. The median spectral energy distributions as well as the values of the derived parameters were compared to those of the local early- and late-type galaxies. In addition to that, (U)LIRGs were divided into seven classes, according to the merging stage of each system, and variations in the derived parameters were investigated.
Results. (U)LIRGs occupy the 'high-end' on the dust mass, stellar mass, and star-formation rate (SFR) plane in the local Universe with median values of 5.2x107 M☉, 6.3x1010M☉, and 52M☉/yr, respectively. The median value of the dust temperature in (U)LIRGs is 32K, which is higher compared to both the early-type (28K) and the late-type (22K) galaxies. The dust emission in PDR regions in (U)LIRGs is 11.7% of the total dust luminosity, which is significantly higher than early-type (1.6%) and late-type (5.2%) galaxies. Small differences in the derived parameters are seen for the seven merging classes of our sample of (U)LIRGs with the most evident one being on the SFR, where in systems in late merging stages ('M3' and 'M4') the median SFR reaches up to 99M☉/yr compared to 26M☉/yr for the isolated ones. In contrast to the local early- and late-type galaxies where the old stars are the dominant source of the stellar emission, the young stars in (U)LIRGs contribute with 64% of their luminosity to the total stellar luminosity. The fraction of the stellar luminosity absorbed by the dust is extremely high in (U)LIRGs (78%) compared to 7% and 25% in early- and late-type galaxies, respectively. The fraction of the stellar luminosity used to heat up the dust grains is very high in (U)LIRGs, for both stellar components (92% and 56% for the young and the old stellar populations, respectively) while 74% of the dust emission comes from the young stars.

Abstract Copyright: © ESO 2021

Journal keyword(s): galaxies: evolution - galaxies: ISM - galaxies: interactions - dust, extinction - galaxies: star formation - galaxies: stellar content

Simbad objects: 78

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Number of rows : 78
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 NGC 17 Sy2 00 11 06.612 -12 06 28.33   14.14 13.52     ~ 369 1
2 MCG-02-01-051 Sy2 00 18 50.898 -10 22 36.49   14.81 14.33     ~ 154 3
3 NGC 232 Sy2 00 42 45.814 -23 33 40.69   14.43   12.78   ~ 167 0
4 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
5 IC 1623 IG 01 07 47.24 -17 30 25.0   15       ~ 338 2
6 MCG-03-04-014 Sy1 01 10 08.92440 -16 51 09.7668   15   13.96   ~ 117 1
7 Z 436-30 LIN 01 20 02.654 +14 21 41.73   14.9       ~ 176 1
8 IRAS 01364-1042 LIN 01 38 52.86288 -10 27 11.5848   16.77   15.74   ~ 132 0
9 ZW III 35 Sy2 01 44 30.516 +17 06 09.18   15.24 14.81     ~ 261 1
10 NGC 695 AGN 01 51 14.3479513536 +22 34 55.956444960   13.7       ~ 201 1
11 NGC 958 Sy2 02 30 42.8187658032 -02 56 20.526742608   13.0   11.81 12.4 ~ 164 0
12 Z 440-4 rG 02 46 17.482 +13 05 44.33   15.2       ~ 141 1
13 UGC 2369 PaG 02 54 00.9 +14 58 31   14.6       ~ 118 1
14 MCG+02-08-029 AGN 02 54 01.80480 +14 58 14.6244           ~ 107 1
15 IRAS 03359+1523 G 03 38 47.1918750504 +15 32 53.853117504   16.3       ~ 112 0
16 Z 418-14 AG? 04 12 22.670 +05 32 49.13   15.50       ~ 170 0
17 ESO 550-25 PaG 04 21 20.00 -18 48 45.8           ~ 65 1
18 NGC 1614 Sy1 04 34 00.027 -08 34 44.57   14.66 13.99     ~ 697 1
19 IRAS 05189-2524 Sy2 05 21 01.3994605776 -25 21 45.321827832   15.47 14.75     ~ 545 0
20 NGC 2146 AGN 06 18 37.710 +78 21 25.27 11.67 11.38 10.59     ~ 765 2
21 NGC 2623 LIN 08 38 24.016 +25 45 16.29 14.10 13.99 13.36     ~ 533 2
22 IRAS 08572+3915 LIN 09 00 25.38288 +39 03 54.2988     16.66     ~ 450 1
23 UGC 4881 IG 09 15 55.5 +44 19 58   14.9       ~ 178 0
24 Z 289-11 Sy2 09 35 51.6045544584 +61 21 11.589382368   15.20 15.50     ~ 617 2
25 Z 239-11 GiP 09 36 30.8337360552 +48 28 10.808036796   15.0       ~ 60 0
26 IC 563 AG? 09 46 20.361 +03 02 43.86   14.7       ~ 101 0
27 NGC 3110 Sy1 10 04 02.12400 -06 28 29.1250   13.4   13.3 12.5 ~ 191 2
28 NVSS J102000+081335 rG 10 20 00.1849825704 +08 13 33.648546108   17.5       ~ 167 1
29 NGC 3256 Sy2 10 27 51.284 -43 54 13.55   11.83 11.33 10.62 11.9 ~ 920 2
30 IRAS 10565+2448 LIN 10 59 18.12811 +24 32 34.7357   15.7       ~ 302 0
31 APG 148 IG 11 03 53.89153 +40 50 59.8850   14.29       ~ 190 1
32 Z 11-76 Sy2 11 21 12.261 -02 59 03.00   15.0       ~ 132 0
33 IC 2810 rG 11 25 45.04728 +14 40 35.8176   15.4       ~ 140 0
34 IC 694 AG? 11 28 27.312 +58 34 42.29   18.2       ~ 258 2
35 NGC 3690 IG 11 28 31.0 +58 33 41   13.19 12.86     ~ 1015 4
36 NAME Antennae IG 12 01 53.170 -18 52 37.92           ~ 1749 0
37 IRAS 12112+0305 PaG 12 13 45.98880 +02 48 39.9600           ~ 373 0
38 [CGM90] IRAS 12112+0305 NE rG 12 13 46.10735 +02 48 41.4959           ~ 369 0
39 6dFGS gJ122503.9-064053 LIN 12 25 03.8941406496 -06 40 52.501670544   15.53       ~ 73 0
40 Z 294-4 Sy1 12 56 14.2341182928 +56 52 25.238373852   14.68 13.84     ~ 2096 3
41 NGC 4922N Sy2 13 01 25.2660290577 +29 18 49.879144069   15.60 14.67 13.85   ~ 265 5
42 MCG-04-31-023 Sy1 13 02 52.3177169808 -23 55 17.932558692   14.77 14.78 13.24 13.59 ~ 131 1
43 IC 860 LIN 13 15 03.51 +24 37 07.8   14.8       ~ 236 0
44 MCG+10-19-056 AGN 13 15 35.103 +62 07 28.43   15       ~ 120 1
45 IC 883 SBG 13 20 35.37960 +34 08 21.8400   14.8       ~ 421 1
46 NGC 5104 AGN 13 21 23.11513 +00 20 33.3820   14.5   13.227   ~ 169 1
47 MCG-03-34-064 Sy2 13 22 24.4583154360 -16 43 42.481822404   14   13.16   ~ 345 2
48 NGC 5135 Sy2 13 25 44.059 -29 50 01.24   12.58 13.35 11.53 12.2 ~ 500 1
49 NGC 5256 PaG 13 38 17.81 +48 16 41.2   14.1 13.42     ~ 449 1
50 NGC 5257 H2G 13 39 52.92781 +00 50 24.0903   13.7 12.99     ~ 208 0
51 NGC 5258 GiP 13 39 57.6768310848 +00 49 51.009668076   13.8 12.83     ~ 186 0
52 Z 271-60 Sy2 13 44 42.1883001099 +55 53 13.596220922   15.68 14.91     ~ 958 3
53 Z 247-20 AGN 14 19 43.2275567784 +49 14 12.014867004   15.4       ~ 141 1
54 LEDA 52270 Sy1 14 37 38.2867288488 -15 00 24.087592692   16.58 16.40     ~ 300 2
55 MCG+04-35-018 GiP 14 57 00.3205510752 +24 36 24.138336996   14.3 15.3     ~ 83 0
56 UGC 9618 IG 14 57 01.0 +24 36 41           ~ 127 0
57 Z 49-57 rG 15 13 13.1083645335 +07 13 32.099256087   15.5       ~ 252 1
58 Z 221-50 SyG 15 18 06.1187 +42 44 45.086   15.0 15     ~ 239 1
59 2MASX J15265942+3558372 LIN 15 26 59.44451 +35 58 37.0521   15.61       ~ 295 1
60 IC 1127 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 3090 4
61 NGC 6090 PaG 16 11 40.3 +52 27 21   14.0       ~ 446 1
62 Z 52-37 AGN 16 30 56.539 +04 04 58.36   14.9       ~ 113 1
63 NGC 6285 AGN 16 58 24.016 +58 57 21.23   15.3       ~ 117 0
64 NGC 6286 AGN 16 58 31.3566512040 +58 56 10.114753560   14.2       ~ 202 1
65 NVSS J171420+531028 rG 17 14 20.4740967144 +53 10 31.495916892           ~ 97 1
66 MCG-03-57-017 Sy1 22 31 25.474 -19 02 04.27   14.27 13.73 12.90   ~ 123 1
67 NAME South America rG 22 51 49.27872 -17 52 24.0600   16.97       ~ 348 3
68 NGC 7469 Sy1 23 03 15.6 +08 52 26 12.60 13.00 12.34     ~ 2253 3
69 IC 5283 GiP 23 03 17.9800776408 +08 53 36.838944528   15.2       ~ 124 1
70 Z 453-62 AGN 23 04 56.514 +19 33 07.86   15.2       ~ 117 0
71 IC 5298 Sy2 23 16 00.6756811155 +25 33 24.081139422   15.0       ~ 205 0
72 NGC 7552 Sy1 23 16 10.66 -42 35 04.7 11.34 11.22 10.57 10.08 11.1 ~ 574 3
73 NGC 7592W Sy2 23 18 21.8077569718 -04 24 56.904279971     15.0     ~ 175 0
74 NGC 7592 IG 23 18 22.2 -04 24 57           ~ 177 0
75 NGC 7674 Sy1 23 27 56.6973043968 +08 46 44.253707772 13.84 13.92 13.23 12.64   ~ 738 2
76 NGC 7770 GiG 23 51 22.610 +20 05 48.56   14.5       ~ 106 1
77 NGC 7771 GiG 23 51 24.880 +20 06 42.57 13.42 13.08 12.25     ~ 350 3
78 Z 455-59 AGN 23 51 26.731 +20 35 10.22   14.9       ~ 237 0

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