2005AJ....129..160S


Query : 2005AJ....129..160S

2005AJ....129..160S - Astron. J., 129, 160-177 (2005/January-0)

DDO 88: a galaxy-sized hole in the interstellar medium.

SIMPSON C.E., HUNTER D.A. and KNEZEK P.M.

Abstract (from CDS):

We present an H I and optical study of the gas-rich dwarf irregular galaxy DDO 88. Although the global optical and H I parameters of DDO 88 are normal for its morphological type, it hosts a large (3 kpc diameter) and unusually complete ring of enhanced H I emission. The normal appearance of this galaxy in the optical and the outer regions of the H I give no hint of the presence of the striking H I ring in the inner regions. The gas ring is located at approximately one-third of the total H I radius and one-half the optically defined Holmberg radius, and contains 30% of the total H I of the galaxy. The ring surrounds a central depression in the H I distribution. If the H I ring and central depression in the gas were formed by the energy input from winds and supernova explosions of massive stars formed in a starburst, as is thought often to be the case, the star-forming event would have formed 0.1%-1% of the total stellar mass of the galaxy. However, the UBV colors in the H I hole are not bluer than the rest of the galaxy, as would be expected if an unusual star-forming event had taken place there recently, although there is an old (∼1-3 Gyr), red cluster near the center of the hole that is massive enough to have produced the hole in the H I. An age estimate for the ring is uncertain, however, because it is not observed to be expanding. An expansion model produces a lower estimate of 0.5 Gyr, but the presence of faint star formation regions associated with the ring indicates a much younger age. We also estimate that the ring could have dispersed by now if it is older than 0.5 Gyr. This implies that the ring is younger than 0.5 Gyr. A younger age would indicate that the red cluster did not produce the hole and ring. Therefore, uncertainties prevent us from concluding that the cluster and the H I hole are definitely related. If this ring and the depression in the gas that it surrounds were not formed by stellar winds and supernovae, this would indicate that some other, currently unidentified, mechanism is operating.

Abstract Copyright:

Journal keyword(s): galaxies: individual (DDO 88) - Galaxies: Irregular - Galaxies: ISM - Galaxies: Kinematics and Dynamics - Galaxies: Photometry

Nomenclature: Table 2, Fig.9: [SHK2005] Region N (Nos 1-5). Text: [SHK2005] Cluster N=1.

Simbad objects: 28

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Number of rows : 28
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 IC 10 G 00 20 25.50 +59 17 17.0   13.6 9.5     ~ 1119 1
2 NGC 206 As* 00 40 33.8 +40 44 22           ~ 127 0
3 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 12651 1
4 NGC 604 HII 01 34 32.1 +30 47 01           ~ 586 0
5 NGC 1156 rG 02 59 42.8528847264 +25 14 28.352017320 12.13 12.32 11.74     ~ 313 1
6 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 17438 0
7 NGC 2363 AG? 07 28 29.59 +69 11 34.3   15.5       ~ 257 1
8 NGC 2363A HII 07 28 42.8 +69 11 21           ~ 564 3
9 NGC 2366 H2G 07 28 52.4529 +69 12 38.859 12.25 11.86 11.39 11.33   ~ 769 0
10 UGC 4305 IG 08 19 04.9864630512 +70 43 13.086910452 12.06 11.72 11.39 11.11   ~ 769 2
11 NAME M 81 Dwarf A G 08 23 55.1 +71 01 56   16.5       ~ 203 1
12 UGC 5139 LSB 09 40 32.33 +71 10 56.0 14.53 14.00 13.66 13.41   ~ 356 1
13 Z 64-73 G 10 08 28.12 +12 18 23.4   11.3 10.0     ~ 1208 1
14 NAME Sex A H2G 10 11 00.5 -04 41 30 12.48 12.13 11.93 11.78   ~ 727 2
15 IC 2574 AG? 10 28 23.6148831408 +68 24 43.440012756 11.70 11.07 10.87 10.74   ~ 665 1
16 [SHK2005] Cluster Cl* 10 47 +14.0           ~ 1 0
17 [SHK2005] Region 2 HII 10 47 +14.0           ~ 1 0
18 [SHK2005] Region 4 HII 10 47 +14.0           ~ 1 0
19 [SHK2005] Region 1 HII 10 47 +14.0           ~ 1 0
20 UGC 5889 GiP 10 47 22.4012897592 +14 04 16.697296020 14.17 14.31 13.61 13.51   ~ 141 1
21 NGC 3377 GiP 10 47 42.400 +13 59 08.30 11.55 11.24 10.38     ~ 775 1
22 NAME M96 Group GrG 10 48 +13.3           ~ 314 0
23 ICRF J112027.8+142054 Sy2 11 20 27.80814059 +14 20 54.9730732   20 20.935 20.100   ~ 167 1
24 UGC 6955 GiG 11 58 29.804 +38 04 34.80   15.2       ~ 79 0
25 NGC 4449 EmG 12 28 11.118 +44 05 36.81 10.11 9.98 9.64 9.45   ~ 1125 1
26 UGC 8024 GiC 12 54 05.248 +27 08 58.67 14.37 14.23 13.95 13.84   ~ 592 1
27 UGC 8320 AG? 13 14 27.997 +45 55 11.14 13.63 13.26 13.02 12.81   ~ 282 0
28 Cul 1328+307 Rad 13 31 08.4 +30 28 37           ~ 7 0

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