2004ApJ...603...82L


Query : 2004ApJ...603...82L

2004ApJ...603...82L - Astrophys. J., 603, 82-86 (2004/March-1)

Globular cluster formation in M82.

LIPSCY S.J. and PLAVCHAN P.

Abstract (from CDS):

We present high-resolution mid-infrared (mid-IR; 11.7 and 17.65 µm) maps of the central 400 pc region of the starburst galaxy M82. Seven star-forming clusters are identified, which together provide ∼15% of the total mid-IR luminosity of the galaxy. We find that these young stellar clusters have inferred masses and sizes comparable to globular clusters. At least 20% of the star formation in M82 is found to occur in super star clusters.

Abstract Copyright: ∼

Journal keyword(s): Galaxies: Individual: Messier Number: M82 - Galaxies: Starburst - Galaxies: Star Clusters - Infrared: Galaxies

Nomenclature: Table 1, Fig.1: [LP2004] A (Nos A-G).

Simbad objects: 15

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Number of rows : 15
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 104 GlC 00 24 05.359 -72 04 53.20     4.09     ~ 4158 0
2 M 81 Sy2 09 55 33.1726556496 +69 03 55.062505368   7.89 6.94     ~ 4725 3
3 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 6156 6
4 * mu. UMa SB* 10 22 19.7276765267 +41 29 58.337745272 6.53 4.64 3.05 1.76 0.80 M0III 331 0
5 NGC 4038 EmG 12 01 53.002 -18 52 03.32   10.91   9.74 11.0 ~ 1364 1
6 NAME Antennae IG 12 01 53.170 -18 52 37.92           ~ 1749 0
7 NGC 4039 GiP 12 01 53.51 -18 53 10.3   11.08   9.77   ~ 1173 1
8 NGC 5139 GlC 13 26 47.28 -47 28 46.1           ~ 3677 0
9 NGC 5253 rG 13 39 55.990 -31 38 24.11 11.48 10.94 10.49 10.33 13.47 ~ 1421 4
10 M 19 GlC 17 02 37.69 -26 16 04.6   8.45 5.57     ~ 406 1
11 * alf Her ** 17 14 38.85818 +14 23 25.2262           M5Ib-II+G5III+F2V: 209 0
12 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
13 NAME Arches Cluster Cl* 17 45 50.5 -28 49 28           ~ 792 0
14 * eta Sgr LP? 18 17 37.6371989461 -36 45 42.084592381 6.37 4.67 3.11 1.55 0.23 M2III 149 0
15 Ass Cyg OB 2 As* 20 33.2 +41 19           ~ 1023 0

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