2011A&A...536A..16P


C.D.S. - SIMBAD4 rel 1.7 - 2020.10.20CEST11:49:37

2011A&A...536A..16P - Astronomy and Astrophysics, volume 536A, 16-16 (2011/12-1)

Planck early results. XVI. The Planck view of nearby galaxies.

PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., ARNAUD M., ASHDOWN M., AUMONT J., BACCIGALUPI C., BALBI A., BANDAY A.J., BARREIRO R.B., BARTLETT J.G., BATTANER E., BENABED K., BENOIT A., BERNARD J.-P., BERSANELLI M., BHATIA R., BOCK J.J., BONALDI A., BOND J.R., BORRILL J., BOUCHET F.R., BUCHER M., BURIGANA C., CABELLA P., CARDOSO J.-F., CATALANO A., CAYON L., CHALLINOR A., CHAMBALLU A., CHARY R.-R., CHIANG L.-Y, CHRISTENSEN P.R., CLEMENTS D.L., COLOMBI S., COUCHOT F., COULAIS A., CRILL B.P., CUTTAIA F., DANESE L., DAVIES R.D., DAVIS R.J., DE BERNARDIS P., DE GASPERIS G., DE ROSA A., DE ZOTTI G., DELABROUILLE J., DELOUIS J.-M., DESERT F.-X., DICKINSON C., DOLE H., DONZELLI S., DORE O., DOERL U., DOUSPIS M., DUPAC X., EFSTATHIOU G., ENSSLIN T.A., FINELLI F., FORNI O., FRAILIS M., FRANCESCHI E., GALEOTTA S., GANGA K., GIARD M., GIARDINO G., GIRAUD-HERAUD Y., GONZALEZ-NUEVO J., GORSKI K.M., GRATTON S., GREGORIO A., GRUPPUSO A., HANSEN F.K., HARRISON D., HELOU G., HENROT-VERSILLE S., HERRANZ D., HILDEBRANDT S.R., HIVON E., HOBSON M., HOLMES W.A., HOVEST W., HOYLAND R.J., HUFFENBERGER K.M., JAFFE A.H., JONES W.C., JUVELA M., KEIHAENEN E., KESKITALO R., KISNER T.S., KNEISSL R., KNOX L., KURKI-SUONIO H., LAGACHE G., LAEHTEENMAEKI A., LAMARRE J.-M., LASENBY A., LAUREIJS R.J., LAWRENCE C.R., LEACH S., LEONARDI R., LINDEN-VORNLE M., LOPEZ-CANIEGO M., LUBIN P.M., MACIAS-PEREZ J.F., MacTAVISH C.J., MADDEN S., MAFFEI B., MAINO D., MANDOLESI N., MANN R., MARIS M., MARTINEZ-GONZALEZ E., MASI S., MATARRESE S., MATTHAI F., MAZZOTTA P., MELCHIORRI A., MENDES L., MENNELLA A., MIVILLE-DESCHENES M.-A., MONETI A., MONTIER L., MORGANTE G., MORTLOCK D., MUNSHI D., MURPHY A., NASELSKY P., NATOLI P., NETTERFIELD C.B., NORGAARD-NIELSEN H.U., NOVIELLO F., NOVIKOV D., NOVIKOV I., OSBORNE S., PAJOT F., PARTRIDGE B., PASIAN F., PATANCHON G., PEEL M., PERDEREAU O., PEROTTO L., PERROTTA F., PIACENTINI F., PIAT M., PLASZCZYNSKI S., POINTECOUTEAU E., POLENTA G., PONTHIEU N., POUTANEN T., PREZEAU G., PRUNET S., PUGET J.-L., REACH W.T., REBOLO R., REINECKE M., RENAULT C., RICCIARDI S., RILLER T., RISTORCELLI I., ROCHA G., ROSSET C., ROWAN-ROBINSON M., RUBINO-MARTIN J.A., RUSHOLME B., SANDRI M., SAVINI G., SCOTT D., SEIFFERT M.D., SHELLARD P., SMOOT G.F., STARCK J.-L., STIVOLI F., STOLYAROV V., SUDIWALA R., SYGNET J.-F., TAUBER J.A., TERENZI L., TOFFOLATTI L., TOMASI M., TORRE J.-P., TRISTRAM M., TUOVINEN J., TUERLER M., UMANA G., VALENZIANO L., VARIS J., VIELVA P., VILLA F., VITTORIO N., WADE L.A., WANDELT B.D., YVON D., ZACCHEI A. and ZONCA A.

Abstract (from CDS):

The all-sky coverage of the Planck Early Release Compact Source Catalogue (ERCSC) provides an unsurpassed survey of galaxies at submillimetre (submm) wavelengths, representing a major improvement in the numbers of galaxies detected, as well as the range of far-IR/submm wavelengths over which they have been observed. We here present the first results on the properties of nearby galaxies using these data. We match the ERCSC catalogue to IRAS-detected galaxies in the Imperial IRAS Faint Source Redshift Catalogue (IIFSCz), so that we can measure the spectral energy distributions (SEDs) of these objects from 60 to 850µm. This produces a list of 1717 galaxies with reliable associations between Planck and IRAS, from which we select a subset of 468 for SED studies, namely those with strong detections in the three highest frequency Planck bands and no evidence of cirrus contamination. The SEDs are fitted using parametric dust models to determine the range of dust temperatures and emissivities. We find evidence for colder dust than has previously been found in external galaxies, with T<20K. Such cold temperatures are found using both the standard single temperature dust model with variable emissivity β, or a two dust temperature model with β fixed at 2. We also compare our results to studies of distant submm galaxies (SMGs) which have been claimed to contain cooler dust than their local counterparts. We find that including our sample of 468 galaxies significantly reduces the distinction between the two populations. Fits to SEDs of selected objects using more sophisticated templates derived from radiative transfer models confirm the presence of the colder dust found through parametric fitting. We thus conclude that cold (T<20K) dust is a significant and largely unexplored component of many nearby galaxies.

Abstract Copyright:

Journal keyword(s): galaxies: photometry - submillimeter: galaxies - infrared: galaxies - galaxies: ISM

Simbad objects: 47

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Number of rows : 47

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 7823 G 00 04 45.596 -62 03 41.47   13.42   12.24   ~ 17 0
2 NGC 157 EmG 00 34 46.751 -08 23 47.36   11.0 19.00 10.03 10.7 ~ 326 0
3 M 31 G 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 11049 1
4 NGC 253 SyG 00 47 33.134 -25 17 19.68   8.03   6.94 8.1 ~ 2954 2
5 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 9554 1
6 IRAS F04257-4913 IR 04 27 05.2 -49 06 54           ~ 1 0
7 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 14984 1
8 QSO B0537-441 BLL 05 38 50.36155219 -44 05 08.9389165   15.77 16.48 16   ~ 792 2
9 FIRST J082621.1+225358 rG 08 26 21.086 +22 53 58.84   15.6       ~ 22 0
10 QSO J0854+2006 BLL 08 54 48.8749311881 +20 06 30.642936668   15.91 15.43 15.56   ~ 2022 1
11 NGC 2905 H2G 09 32 10.111 +21 30 02.99 10.44 9.75 9.07 8.68   ~ 997 3
12 NGC 3049 EmG 09 54 49.651 +09 16 17.90   13.04       ~ 292 1
13 M 82 IG 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 5367 6
14 NGC 3259 Sy1 10 32 34.8644758319 +65 02 27.928044793   17.55 16.89     ~ 139 0
15 IRAS F10361+4155 IR 10 39 02.6 +41 40 21           ~ 2 0
16 NGC 3810 GiG 11 40 58.737 +11 28 16.07   11.4       ~ 306 1
17 NGC 3938 GiG 11 52 49.453 +44 07 14.63 10.80 10.90 10.38     ~ 471 1
18 UGC 6930 EmG 11 57 17.395 +49 16 59.71   14.2       ~ 104 0
19 NGC 4096 GiG 12 06 01.161 +47 28 42.09   11.61   10.86   ~ 222 0
20 NGC 4274 LIN 12 19 50.665 +29 36 52.92 11.78 11.34 10.41     ~ 226 1
21 M 100 AGN 12 22 54.9318850854 +15 49 20.294302163 10.04 10.05 9.35     ~ 1668 2
22 3C 273 BLL 12 29 06.6996828061 +02 03 08.598846466   13.05 14.830 14.11   ~ 5348 1
23 3C 279 QSO 12 56 11.1664521013 -05 47 21.531840471   18.01 17.75 15.87   ~ 2725 2
24 Mrk 231 Sy1 12 56 14.2340989340 +56 52 25.238555193   14.68 13.84     ~ 1791 3
25 M 51 GiP 13 29 52.698 +47 11 42.93   9.26 8.36 8.40   ~ 3833 4
26 UGC 8684 GiG 13 42 15.916 +60 46 36.39   14.5       ~ 54 0
27 IRAS F13443+4407 IR 13 46 23.2 +43 52 27           ~ 1 0
28 NGC 5297 GiP 13 46 23.694 +43 52 19.34   12.3       ~ 144 0
29 NGC 5334 LSB 13 52 54.4632693594 -01 06 52.601149767   12.0   12.3 12.1 ~ 151 0
30 NGC 5362 GiG 13 54 53.298 +41 18 48.72   13.2   12.17   ~ 76 0
31 IRAS F14004+5603 IR 14 02 10.5 +55 48 53           ~ 1 0
32 IC 979 LIN 14 09 32.3664353130 +14 49 54.599419301   14.5       ~ 21 0
33 NGC 5529 GiP 14 15 34.226 +36 13 37.12   12.9       ~ 141 2
34 IRAS F14134+3627 IR 14 15 34.9 +36 13 32           ~ 1 0
35 NGC 5669 H2G 14 32 43.476 +09 53 25.47   13.2       ~ 166 0
36 NGC 5676 GiG 14 32 46.853 +49 27 28.11   11.7       ~ 233 1
37 NGC 5701 GiG 14 39 11.0762411300 +05 21 48.498854025 12.03 11.76 10.88     ~ 224 1
38 NGC 5874 GiG 15 07 51.820 +54 45 10.08   14.1       ~ 82 0
39 Mrk 847 G 15 13 29.224 +58 30 33.22   15.0       ~ 20 0
40 UGC 9853 LIN 15 25 46.798 +52 26 41.37   15.10       ~ 49 0
41 UGC 9858 GiG 15 26 41.481 +40 33 51.84   14.0       ~ 82 0
42 IC 4553 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 2701 4
43 NVSS J155041+553639 rG 15 50 42.1367620453 +55 36 38.467231050   15.4       ~ 19 0
44 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11754 0
45 M 2 GlC 21 33 27.02 -00 49 23.7     6.25     ~ 906 1
46 NGC 7537 GiP 23 14 34.515 +04 29 54.43   13.8       ~ 199 0
47 NGC 7541 GiP 23 14 43.857 +04 32 02.04   12.7       ~ 296 1

    Equat.    Gal    SGal    Ecl

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2020.10.20-11:49:37

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