2005PASJ...57..549T


Query : 2005PASJ...57..549T

2005PASJ...57..549T - Publ. Astron. Soc. Jap., 57, 549-561 (2005/August-0)

High angular resolution observations of the (J,K) = (1,1), (2,2) and (3.3) transitions of ammonia in NGC 253.

TAKANO S., HOFNER P., WINNEWISSER G., NAKAI N. and KAWAGUCHI K.

Abstract (from CDS):

The nearby starburst galaxy NGC 253 was mapped in the ammonia (J, K) = (1, 1), (2, 2), and (3, 3) lines in the 23GHz region with the Very Large Array. The angular resolutions were about 4'' * 3''. The distributions of the three lines were different from one another. The (1, 1) and (3, 3) lines were distributed along the bar mainly at the northeastern and southwestern regions from the center, but the (2, 2) line is distributed mainly at two clumps in the southwestern region from the center. In addition, the (1, 1) line showed absorption at the central region. The obtained rotational temperatures were < 15–28 K (lower limit), depending on the clumps. The ammonia distributions are generally consistent with estimates from our single-dish results already published. The distributions of ammonia were compared with those of continuum and several other molecular lines.

Abstract Copyright: ∼

Journal keyword(s): galaxies: individual: NGC 253 - galaxies: starburst - ISM: molecules - molecular processes - radio lines: galaxies

Nomenclature: Fig.6, Table 2: [THW2005] WWN (Nos NE1-NE2, SW1-SW2).

Simbad objects: 6

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Number of rows : 6
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 [AU88] 5.48-43.3 SNR 00 47 32.88 -25 17 21.5           ~ 17 0
2 NGC 253 SyG 00 47 33.134 -25 17 19.68   8.03   6.94 8.1 ~ 3588 2
3 QSO B0118-272 BLL 01 20 31.6628068344 -27 01 24.636341064   15.89 15.56 15.49   ~ 288 1
4 3C 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2924 2
5 NGC 1275 Bla 03 19 48.1599902040 +41 30 42.108850836   13.10 12.48 11.09   ~ 4243 3
6 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 6156 6

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