2001A&A...370...34R


C.D.S. - SIMBAD4 rel 1.7 - 2020.11.28CET13:27:03

2001A&A...370...34R - Astronomy and Astrophysics, volume 370, 34-42 (2001/4-4)

IC 10: More evidence that it is a blue compact dwarf.

RICHER M.G., BULLEJOS A., BORISSOVA J., McCALL M.L., LEE H., KURTEV R., GEORGIEV L., KINGSBURGH R.L., ROSS R. and ROSADO M.

Abstract (from CDS):

We present optical spectroscopy of HII regions in the Local Group galaxy IC 10 and UBVR photometry of foreground stars in three fields towards this galaxy. From these data, we find that the foreground reddening due to the Milky Way is E(B-V)=0.77±0.07mag. We find that IC 10 contains considerable internal dust, which qualitatively explains the variety of reddening values found by studies of its different stellar populations. Based upon our foreground reddening, IC 10 has intrinsic photometric properties like those of a blue compact dwarf galaxy, and not those of a dwarf irregular. This result is consistent with much evidence that IC 10 is in the throes of a starburst that began at least 10Myr ago. We also report the discovery of a new WR star in the HII region HL111c.

Abstract Copyright:

Journal keyword(s): galaxies: individual: IC 10 - galaxies: local group - galaxies: fundamental parameters - galaxies: starburst - galaxies: dwarf

Simbad objects: 25

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Number of rows : 25

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 [HL90] 30 HII 00 20 12.7 +59 20 22           ~ 5 0
2 [BGR2000] Br 1 HII 00 20 17.4 +59 18 40           ~ 14 0
3 [BGR2000] Br 2 SNR 00 20 19.12 +59 18 53.5           ~ 12 0
4 [HL90] 77 HII 00 20 22.4 +59 17 52           ~ 3 0
5 [HL90] 81 HII 00 20 22.9 +59 17 16           ~ 2 0
6 IC 10 G 00 20 23.16 +59 17 34.7   13.6 9.5     ~ 1017 0
7 [BGR2000] Br 5 HII 00 20 25.6 +59 17 26           ~ 10 0
8 [HL90] 111b HII 00 20 26.0 +59 17 42           ~ 9 0
9 [HL90] 111c HII 00 20 26.3 +59 17 57           ~ 16 0
10 [BGR2000] Br 6 HII 00 20 26.5 +59 17 30           ~ 9 0
11 [HL90] 111e HII 00 20 26.7 +59 17 52           ~ 8 0
12 [HL90] 111d HII 00 20 27.2 +59 17 53           ~ 12 0
13 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 9607 1
14 Hilt 102 * 01 09 05.0413010293 +62 47 30.265788867 10.88 11.10 10.42     B0III 46 0
15 HD 19445 PM* 03 08 25.5884 +26 19 51.400 8.29 8.52 8.06 7.60 7.27 G2VFe-3 742 0
16 HD 289002 * 06 45 13.3726265810 +02 08 14.688016523 10.06 10.62 10.44     B1 232 0
17 HD 74721 HB* 08 45 59.2617958540 +13 15 48.592813847 8.88 8.75 8.72     A0V 139 0
18 M 81 Sy2 09 55 33.17306143 +69 03 55.0609270   7.89 6.94     ~ 4009 5
19 HD 109995 HB* 12 38 47.5986540271 +39 18 31.629329712 7.83 7.68   7.6   A0V 215 0
20 M 101 GiP 14 03 12.583 +54 20 55.50   8.46 7.86 7.76   ~ 2579 2
21 * alf Lyr dS* 18 36 56.33635 +38 47 01.2802 0.03 0.03 0.03 0.07 0.10 A0Va 2526 0
22 BD+28 4211 HS* 21 51 11.0220905905 +28 51 50.366090892 8.922 10.25 10.58 10.656 10.831 sdO2VIIIHe5 740 0
23 LP 877-23 PM* 22 52 41.0353308036 -20 35 32.995847106   13.02 11.90     ~ 104 0
24 ESO 191-2 IG 22 53 39.1 -53 22 07           ~ 3 0
25 HD 217086 Y*O 22 56 47.1887219290 +62 43 37.654789076 7.88 8.30 7.66 8.35   O7Vnn((f))z 244 0

    Equat.    Gal    SGal    Ecl

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2020.11.28-13:27:04

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