2020ApJ...888...92L


Query : 2020ApJ...888...92L

2020ApJ...888...92L - Astrophys. J., 888, 92-92 (2020/January-2)

Star-forming clumps in local luminous infrared galaxies.

LARSON K.L., DIAZ-SANTOS T., ARMUS L., PRIVON G.C., LINDEN S.T., EVANS A.S., HOWELL J., CHARMANDARIS V., U V., SANDERS D.B., STIERWALT S., BARCOS-MUNOZ L., RICH J., MEDLING A., COOK D., OKLOPCIC A., MURPHY E.J. and BONFINI P.

Abstract (from CDS):

We present HST narrowband near-infrared imaging of Paα and Paβ emission of 48 local luminous infrared galaxies (LIRGs) from the Great Observatories All-Sky LIRG Survey. These data allow us to measure the properties of 810 spatially resolved star-forming regions (59 nuclei and 751 extranuclear clumps) and directly compare their properties to those found in both local and high-redshift star-forming galaxies. We find that in LIRGs the star-forming clumps have radii ranging from ∼90 to 900 pc and star formation rates (SFRs) of ∼1 x 10–3 to 10 M yr–1, with median values for extranuclear clumps of 170 pc and 0.03 M yr–1. The detected star-forming clumps are young, with a median stellar age of 8.7 Myr, and have a median stellar mass of 5 x 105 M. The SFRs span the range of those found in normal local star-forming galaxies to those found in high-redshift star-forming galaxies at z = 1-3. The luminosity function of the LIRG clumps has a flatter slope than found in lower-luminosity, star-forming galaxies, indicating a relative excess of luminous star-forming clumps. In order to predict the possible range of star-forming histories and gas fractions, we compare the star-forming clumps to those measured in the MassiveFIRE high-resolution cosmological simulation. The star-forming clumps in MassiveFIRE cover the same range of SFRs and sizes found in the local LIRGs and have total gas fractions that extend from 10% to 90%. If local LIRGs are similar to these simulated galaxies, we expect that future observations with ALMA will find a large range of gas fractions, and corresponding star formation efficiencies, among the star-forming clumps in LIRGs.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Interacting galaxies - Star-forming regions - Luminous infrared galaxies

VizieR on-line data: <Available at CDS (J/ApJ/888/92): table1.dat table3.dat>

Status at CDS : Examining the need for a new acronym.

Simbad objects: 52

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Number of rows : 52
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 NGC 23 AG? 00 09 53.411 +25 55 25.46   12.5       ~ 313 3
2 MCG-02-01-051 Sy2 00 18 50.898 -10 22 36.49   14.81 14.33     ~ 141 3
3 MCG+12-02-001 AG? 00 54 03.943 +73 05 05.23   16       ~ 109 1
4 NGC 633 EmG 01 36 23.418 -37 19 17.64   13.50   12.50   ~ 93 1
5 IC 214 G 02 14 05.586 +05 10 23.37   14.4       ~ 149 0
6 UGC 1845 GiG 02 24 07.9838118384 +47 58 10.747047684   15.7       ~ 85 1
7 IRAS 02438+2122 GiG 02 46 39.192 +21 35 09.38   16.0       ~ 73 0
8 IRAS 03217+4023 GiG 03 25 05.3343453936 +40 33 30.822573924           ~ 47 0
9 NAME Hubble Ultra Deep Field reg 03 32 39.0 -27 47 29           ~ 1666 0
10 2MASX J04023209+6020377 G 04 02 32.098 +60 20 37.79           ~ 42 0
11 NGC 1614 Sy1 04 34 00.027 -08 34 44.57   14.66 13.99     ~ 667 0
12 2MASX J05165609+5131561 G 05 16 56.091 +51 31 56.17           ~ 37 0
13 UGC 3351 Sy2 05 45 47.836 +58 42 03.83   16.0       ~ 101 2
14 NGC 2369 Sy1 07 16 37.753 -62 20 37.51   13.23   11.56 12.3 ~ 130 0
15 NGC 2388 GiG 07 28 53.4535009080 +33 49 08.554343196   14.7       ~ 135 2
16 MCG+02-20-003 GiG 07 35 43.416 +11 42 35.29   15.0       ~ 73 0
17 2MASX J08370182-4954302 G 08 37 01.827 -49 54 30.27           ~ 59 0
18 NGC 3110 Sy1 10 04 02.0 -06 28 29   13.4   13.3 12.5 ~ 174 3
19 IC 2545 Sy1 10 06 04.581 -33 53 05.55   15.27 14.27 14.25   ~ 111 0
20 NGC 3256 Sy2 10 27 51.284 -43 54 13.55   11.83 11.33 10.62 11.9 ~ 848 2
21 ESO 320-30 EmG 11 53 11.722 -39 07 48.72   13.30   11.86   ~ 186 1
22 NGC 4922 SyG 13 01 25.2660290577 +29 18 49.879144069   15.60 14.67 13.85   ~ 253 5
23 MCG-02-33-098 AG? 13 02 19.5 -15 46 05   14       ~ 89 0
24 IC 860 LIN 13 15 03.51 +24 37 07.8   14.8       ~ 217 0
25 2MASX J13150638-5509225 Sy2 13 15 06.383 -55 09 22.60   17.3       ~ 147 0
26 IC 883 SBG 13 20 35.4 +34 08 22   14.8       ~ 400 1
27 NGC 5135 Sy2 13 25 44.059 -29 50 01.24   12.58 13.35 11.53 12.2 ~ 474 1
28 NGC 5257 H2G 13 39 52.273 +00 50 22.48   13.7 12.99     ~ 197 0
29 NGC 5258 GiP 13 39 57.6768310848 +00 49 51.009668076   13.8 12.83     ~ 174 0
30 NGC 5331 GiP 13 52 16.289 +02 06 04.18           ~ 90 0
31 NGC 5734 Sy2 14 45 09.0364267176 -20 52 13.484556696   13.75   12.08   ~ 81 1
32 UGC 9618 S GiP 14 57 00.3205510752 +24 36 24.138336996   14.3 15.3     ~ 74 2
33 UGC 9618 IG 14 57 00.4 +24 36 44   14.3       ~ 122 1
34 IC 4518 Sy2 14 57 45.6 -43 07 58   14.5       ~ 74 0
35 ESO 99-4 G 15 24 58.217 -63 07 34.43   16.4       ~ 44 0
36 NGC 5936 H2G 15 30 00.846 +12 59 21.55   13.0       ~ 167 1
37 NGC 6090 PaG 16 11 40.3 +52 27 21   14.0       ~ 430 2
38 IRAS 16164-0746 Sy1 16 19 11.792 -07 54 02.61   15.49       ~ 79 0
39 LEDA 58817 Sy1 16 42 40.1747908920 -09 43 18.848119476   16.77       ~ 98 0
40 NGC 6240 Sy2 16 52 58.9 +02 24 03   14.31 13.37     ~ 1637 2
41 IRAS 17138-1017 Sy2 17 16 35.83992 -10 20 38.9832   17.43   14.59   ~ 131 0
42 IC 4686 AG? 18 13 38.7810951072 -57 43 57.306382932   14.67   13.52   ~ 67 1
43 IC 4687 AGN 18 13 39.829 -57 43 31.25   14.35 14.3 12.78   ~ 136 1
44 IC 4734 GiG 18 38 25.6846404504 -57 29 25.078201116   14.21   12.71   ~ 85 0
45 NGC 6701 AG? 18 43 12.429 +60 39 12.13   12.9       ~ 133 1
46 NGC 6786 Sy2 19 10 53.928 +73 24 36.20   13.7       ~ 72 1
47 NGC 7130 Sy2 21 48 19.5412287192 -34 57 04.492024884   12.86 13.87 11.57   ~ 450 0
48 IC 5179 Sy1 22 16 09.1191653256 -36 50 37.117603752   12.29 11.89 11.38   ~ 204 1
49 NGC 7469 Sy1 23 03 15.6 +08 52 26 12.60 13.00 12.34     ~ 2095 3
50 NGC 7591 SyG 23 18 16.2727927344 +06 35 09.108933504   13.8       ~ 269 0
51 LEDA 90436 G 23 46 05.7217380192 +53 13 56.609577840           ~ 53 0
52 NGC 7771 GiG 23 51 24.880 +20 06 42.57 13.42 13.08 12.25     ~ 338 4

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