2003A&A...410...83H


C.D.S. - SIMBAD4 rel 1.7 - 2021.03.03CET03:17:17

2003A&A...410...83H - Astronomy and Astrophysics, volume 410, 83-100 (2003/10-4)

Star formation rate in galaxies from UV, IR, and Hα estimators.

HIRASHITA H., BUAT V. and INOUE A.K.

Abstract (from CDS):

Infrared (IR) luminosity of galaxies originating from dust thermal emission can be used as an indicator of the star formation rate (SFR). Inoue et al. (2000PASJ...52..539I, IHK) have derived a formula for the conversion from dust IR luminosity to SFR by using the following three quantities: the fraction of Lyman continuum luminosity absorbed by gas (f), the fraction of UV luminosity absorbed by dust (ε), and the fraction of dust heating from old (>108yr) stellar populations (η). We develop a method to estimate those three quantities based on the idea that the various way of SFR estimates from ultraviolet (UV) luminosity (2000Å luminosity), Hα luminosity, and dust IR luminosity should return the same SFR. After applying our method to samples of galaxies, the following results are obtained in our framework. First, our method is applied to a sample of star-forming galaxies, finding that f∼0.6, ε∼0.5, and η∼0.4 as representative values. Next, we apply the method to a starburst sample, which shows larger extinction than the star-forming galaxy sample. With the aid of f, ε, and η, we are able to estimate reliable SFRs from UV and/or IR luminosities. Moreover, the Hα luminosity, if the Hα extinction is corrected by using the Balmer decrement, is suitable for a statistical analysis of SFR, because the same correction factor for the Lyman continuum extinction (i.e. 1/f) is applicable to both normal and starburst galaxies over all the range of SFR. The metallicity dependence of f and ε is also tested: Only the latter proves to have a correlation with metallicity. As an extension of our result, the local (z=0) comoving density of SFR can be estimated with our dust extinction corrections. We show that all UV, Hα, and IR comoving luminosity densities at z=0 give a consistent SFR per comoving volume (∼3x10–2hM/yr/Mpc3). Useful formulae for SFR estimate are listed.

Abstract Copyright:

Journal keyword(s): ISM: dust, extinction - galaxies: evolution - galaxies: ISM - galaxies: starburst - infrared: galaxies - ultraviolet: galaxies

Simbad objects: 53

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Number of rows : 53

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 IC 1586 bCG 00 47 56.301 +22 22 22.51   15.0       ~ 68 0
2 Mrk 960 bCG 00 48 35.430 -12 42 59.77   15.5       ~ 102 0
3 Mrk 357 SyG 01 22 40.5869519680 +23 10 14.696079946   15.76 15.40     ~ 92 0
4 IC 214 G 02 14 05.586 +05 10 23.37   14.4       ~ 140 0
5 NGC 1140 EmG 02 54 33.5258827369 -10 01 43.135585379 12.41 12.84 12.49 13.6 13.5 ~ 267 1
6 NGC 1510 GiP 04 03 32.640 -43 24 00.58 14.23 13.63 13.24 13.09   ~ 179 1
7 NGC 1614 AGN 04 34 00.027 -08 34 44.57   14.66 13.99     ~ 611 0
8 UGC 4308 AGN 08 17 25.776 +21 41 08.06   14.5       ~ 91 0
9 UGC 4324 GiG 08 18 29.5552893125 +20 45 40.902810214   15.3       ~ 64 0
10 2MASX J08184909+2113053 GiG 08 18 49.100 +21 13 05.35   15.5       ~ 38 0
11 UGC 4329 LSB 08 19 01.8842047608 +21 11 09.015839671   15.0       ~ 88 0
12 NVSS J081904+214730 rG 08 19 05.0924503501 +21 47 29.056119837   15.2       ~ 47 0
13 IC 2293 GiG 08 19 32.1130216817 +21 23 39.505540106   15.2       ~ 31 0
14 2MASX J08195880+2103581 GiG 08 19 58.804 +21 03 58.15   15.7       ~ 43 0
15 NGC 3125 H2G 10 06 33.318 -29 56 07.32 13.03 13.45 13.00 12.50 13.4 ~ 217 1
16 NGC 4152 AGN 12 10 37.511 +16 01 58.56   14.00 13.35     ~ 218 0
17 MCG+03-31-063 LIN 12 11 21.9645970669 +19 05 18.442918257   15.3       ~ 24 0
18 NGC 4178 H2G 12 12 46.443 +10 51 57.59   12.9       ~ 324 0
19 NGC 4189 GiG 12 13 47.278 +13 25 29.45   12.51 11.74     ~ 253 1
20 M 98 LIN 12 13 48.292 +14 54 01.69 11.25 10.95 10.14     ~ 451 1
21 NGC 4194 AGN 12 14 09.615 +54 31 35.93   13.79 13.30     ~ 419 2
22 IC 3061 GiG 12 15 04.519 +14 01 44.31   14.9       ~ 134 0
23 M 99 H2G 12 18 49.625 +14 24 59.36 10.45 10.44 9.87     ~ 789 2
24 IC 776 EmG 12 19 03.119 +08 51 22.15   14.9       ~ 124 0
25 Z 99-22 bCG 12 21 11.2538430522 +17 38 19.506504841   14.9       ~ 62 0
26 IC 3258 GiC 12 23 44.495 +12 28 42.06   14.3       ~ 141 0
27 NGC 4351 GiG 12 24 01.560 +12 12 18.09   13.5       ~ 197 0
28 NGC 4383 AGN 12 25 25.518 +16 28 12.02 12.41 12.67 12.12     ~ 227 1
29 UGC 7513 GiG 12 25 42.634 +07 13 00.15   14.4       ~ 162 0
30 NGC 4388 Sy2 12 25 46.820 +12 39 43.45 11.91 11.76 11.02     ~ 1217 2
31 NGC 4416 GiG 12 26 46.720 +07 55 07.80   13.15 11.57     ~ 153 0
32 IC 3414 GiG 12 29 28.7707880441 +06 46 18.549648514   14.2       ~ 101 0
33 NGC 4470 H2G 12 29 37.8070254595 +07 49 27.286182613   12.9       ~ 205 0
34 NGC 4498 GiP 12 31 39.5598460639 +16 51 09.626835314   12.8       ~ 207 0
35 IC 3476 GiG 12 32 41.744 +14 03 05.81   13.5       ~ 169 0
36 NGC 4532 GiP 12 34 19.329 +06 28 03.73   12.3       ~ 256 2
37 IC 3576 AGN 12 36 37.675 +06 37 15.19   15.90 15.40     ~ 105 1
38 NGC 4651 LIN 12 43 42.627 +16 23 36.23   11.30 10.92 10.42 9.84 ~ 471 0
39 NGC 4848 AGN 12 58 05.5774186519 +28 14 33.264194270   14.2   13.53   ~ 175 0
40 Mrk 57 EmG 12 58 37.282 +27 10 35.81   15.88   14.82   ~ 97 0
41 IC 4040 rG 13 00 37.861 +28 03 28.68 15.13 15.1 14.76 14.708 13.981 ~ 146 0
42 MCG+05-31-133 SBG 13 06 38.141 +28 50 56.12   15.19 14.83 13.15   ~ 71 0
43 Mrk 66 Sy2 13 25 53.813 +57 15 16.08   15.0       ~ 74 0
44 Mrk 829 GiP 14 50 56.495 +35 34 18.27   14.5 14.83     ~ 195 0
45 NGC 5860 EmG 15 06 33.73 +42 38 29.2   14.2       ~ 83 0
46 UGC 10033 IG 15 46 56.1 +17 52 42           ~ 114 0
47 NGC 5996 H2G 15 46 58.872 +17 53 03.18   13.2       ~ 143 0
48 NGC 6052 IG 16 05 12.8707837896 +20 32 32.613940524 13.01 13.44 13.00     ~ 336 2
49 NGC 6090 PaG 16 11 40.3 +52 27 21   14.0       ~ 402 2
50 Mrk 499 bCG 16 48 24.1214564075 +48 42 32.774673496   14.6       ~ 47 0
51 ESO 338-4 IG 19 27 58.338 -41 34 30.81   13.55 13.21 13.14 13.43 ~ 212 1
52 NGC 7250 G 22 18 17.776 +40 33 44.66 13.18 13.22 12.58     ~ 90 1
53 NGC 7673 EmG 23 27 41.060 +23 35 20.18 12.84 13.17 12.76     ~ 264 1

    Equat.    Gal    SGal    Ecl

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2021.03.03-03:17:17

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