2009MNRAS.395.2045V


Query : 2009MNRAS.395.2045V

2009MNRAS.395.2045V - Mon. Not. R. Astron. Soc., 395, 2045-2055 (2009/June-1)

Multifrequency study of the ring nebula SG13.

VASQUEZ J., CAPPA C.E. and PINEAULT S.

Abstract (from CDS):

We investigate the morphology and kinematics of the interstellar medium in the environs of the open cluster Mrk50, which includes the Wolf-Rayet star WR157 and a number of early B-type stars. The analysis was performed using radio continuum images at 408 and 1420 MHz, and Hi 21-cm line data taken from the Canadian Galactic Plane Survey, molecular observations of the 12CO (J = 1 ⟶ 0) line at 115 GHz from the Five College Radio Astronomy Observatory and available mid- and far-infrared (FIR) observations obtained with the Midcourse Space Experiment and IRAS satellites, respectively.

This study allowed the identification of the radio continuum and molecular counterpart of the ring nebula SG13, while no neutral atomic structure was found to be associated. The nebula is also detected in the images in the mid- and FIR, showing the existence of dust well mixed with the ionized gas. We estimate the main physical parameters of the material linked to the nebula.

The interstellar gas distribution in the environs of Mrk50 is compatible with a stellar wind bubble created by the mass loss from WR157.

The distribution of young stellar object candidates in the region shows that the stellar formation activity may be present in the molecular shell that encircles the ring nebula.


Abstract Copyright: © 2009 The Authors. Journal compilation © 2009 RAS

Journal keyword(s): stars: Wolf-Rayet - ISM: bubbles - Hii regions

Simbad objects: 38

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Number of rows : 38
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 NAME Per Arm PoG 03 30 +45.0           ~ 1672 0
2 IRAS 23088+6014 LP* 23 11 07.0286952072 +60 31 43.602216204           ~ 16 1
3 2MASS J23120304+6018385 LP? 23 12 03.0297540840 +60 18 38.514653640           ~ 2 0
4 UCAC3 302-174116 * 23 12 12.4968019440 +60 39 49.668272568           ~ 2 0
5 2MASS J23122993+6007256 Y*? 23 12 29.9390477208 +60 07 25.595802840           ~ 1 0
6 2MASS J23125722+6027223 Y*? 23 12 57.2309001984 +60 27 22.309407180           ~ 1 0
7 NVSS J231310+601236 Rad 23 13 10.95 +60 12 36.1           ~ 1 0
8 TYC 4279-2575-1 * 23 13 16.5027314136 +60 19 05.697238188   12.60 12.76     ~ 1 0
9 TYC 4279-910-1 * 23 13 26.9699849160 +60 03 57.005931168   12.38 12.34     A0 2 0
10 IRAS 23113+6027 * 23 13 27.5395199136 +60 43 47.293581900           ~ 5 0
11 2MASS J23133130+6017273 Em* 23 13 31.3042114080 +60 17 27.302489160           ~ 4 0
12 2MASS J23134236+6031201 Y*? 23 13 42.3640255968 +60 31 20.107938072           ~ 1 0
13 1WGA J2313.8+6024 X 23 13 48.8 +60 24 06           ~ 1 0
14 BD+59 2675 * 23 14 11.3020253568 +60 23 10.787259804   10.92 10.34     B8 12 0
15 TYC 4279-1351-1 * 23 14 24.9072252096 +60 13 42.099588444   12.97 12.24     ~ 1 0
16 2MASS J23144274+6043428 Y*? 23 14 42.7670509848 +60 43 42.804763896           ~ 1 0
17 SIM 13 Rad 23 14.8 +60 11           ~ 3 1
18 2MASS J23145423+6034254 Y*? 23 14 54.2344297488 +60 34 25.431363444           ~ 1 0
19 HD 219460 ** 23 15 12.39033 +60 27 01.8129 10.23 10.51 9.89 9.563   B1II+WN4.5 135 0
20 HD 219460A * 23 15 12.3995306290 +60 27 01.845560649   10.97 10.57     B0.7II 128 0
21 Cl Mrk 50 OpC 23 15 14.5 +60 26 25   9.09 8.5     ~ 56 0
22 SH 2-159 Y*O 23 15 31.2384366062 +61 07 10.181362705           ~ 188 1
23 LBN 111.14-00.72 HII 23 16 03.94 +60 02 00.9           ~ 102 2
24 SH 2-157 A HII 23 16.1 +60 02           ~ 10 0
25 2MASS J23161127+6001148 Y*? 23 16 11.2852302336 +60 01 14.808988956           ~ 1 0
26 IRAS 23141+6030 IR 23 16 19.8 +60 47 06           ~ 6 0
27 IRAS 23141+6008 IR 23 16 21.1 +60 25 06           ~ 3 0
28 IRAS 23143+6036 FIR 23 16 29.5 +60 53 20           ~ 3 0
29 2MASS J23164107+6011498 Y*? 23 16 41.0776581768 +60 11 49.910314848           ~ 1 0
30 2MASS J23164539+6035553 Y*? 23 16 45.3900587448 +60 35 55.289206716           ~ 2 0
31 2MASS J23164590+6049490 Y*? 23 16 45.904 +60 49 49.04           ~ 1 0
32 2MASS J23164713+6010319 Y*? 23 16 47.1241169136 +60 10 31.954251036           ~ 1 0
33 IRAS 23146+6022 FIR 23 16 47.8 +60 38 37           ~ 3 0
34 IRAS 23146+5954 IR 23 16 48.9 +60 10 46           ~ 20 0
35 IRAS 23151+6026 FIR 23 17 18.5 +60 42 41           ~ 3 0
36 EM* MWC 1080 Ae* 23 17 25.5895018656 +60 50 43.444557384   13.24 11.85 11.251   B0eq 331 0
37 TYC 4279-2211-1 * 23 17 37.1348509104 +60 27 40.829119992   10.72 10.40     A3 2 0
38 NAME Cas A SNR 23 23 26.0 +58 48 41     14.30     ~ 3033 1

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