2005ApJS..156..179D


Query : 2005ApJS..156..179D

2005ApJS..156..179D - Astrophys. J., Suppl. Ser., 156, 179-215 (2005/February-0)

Observations of massive star-forming regions with water masers: mid-infrared imaging.

DE BUIZER J.M., RADOMSKI J.T., TELESCO C.M. and PINA R.K.

Abstract (from CDS):

We present here a mid-infrared imaging survey of 26 sites of water maser emission. Observations were obtained at the Infrared Telescope Facility 3 m telescope with the University of Florida mid-infrared imager/spectrometer OSCIR, and the JPL mid-infrared camera MIRLIN. The main purpose of the survey was to explore the relationship between water masers and the massive star formation process. It is generally believed that water masers predominantly trace outflows and embedded massive stellar objects, but may also exist in circumstellar disks around young stars. We investigate each of these possibilities in light of our mid-infrared imaging. We find that mid-infrared emission seems to be more closely associated with water and OH maser emission than cm radio continuum emission from UC H II regions. We also find from the sample of sources in our survey that, like groups of methanol masers, both water and OH masers have a proclivity for grouping into linear or elongated distributions. We conclude that the vast majority of linearly distributed masers are not tracing circumstellar disks, but outflows and shocks instead.

Abstract Copyright: ∼

Journal keyword(s): Stars: Circumstellar Matter - Infrared: Stars - Masers - Stars: Formation

Nomenclature: Table 2: DRT05 GLL.ll+B.bb N N=28, DRT05 Cep A HW 2 N N=1.

Status at CDS : All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 93

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Number of rows : 93
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 W 3 IRS 5 Cluster Cl* 02 25 42 +62 06.1           ~ 83 1
2 NAME W 3 OH HII 02 27 04.1 +61 52 22           ~ 1064 2
3 NGC 2071 RNe 05 47 10 +00 18.0           ~ 661 1
4 OH 000.38+00.04 Mas 17 46 21.4012 -28 35 39.821           ~ 22 0
5 IRAS 17432-2835 HII 17 46 27.4 -28 36 06           ~ 29 0
6 OH 000.55-00.85 Mas 17 50 14.35 -28 54 31.1           ~ 34 0
7 RCW 142 HII 17 50 15.3 -28 54 03           ~ 64 0
8 [GRM93] G09.61+0.20 A Rad 18 06 11.9 -20 31 41           ~ 15 0
9 DRT03 G09.62+0.19 1 IR 18 06 13.4330 -20 31 28.000           ~ 2 0
10 DRT03 G09.62+0.19 2 IR 18 06 13.8530 -20 31 26.500           ~ 2 0
11 GAL 009.62+00.19 HII 18 06 13.9 -20 31 44           ~ 226 0
12 [GRM93] G09.61+0.20 B Rad 18 06 14.1 -20 31 43           ~ 19 0
13 DRT03 G09.62+0.19 3 IR 18 06 14.2470 -20 31 46.100           ~ 2 0
14 DRT03 G09.62+0.19 4 IR 18 06 14.3670 -20 31 25.800           ~ 2 0
15 [GRM93] G09.61+0.20 C HII 18 06 14.4 -20 31 25           ~ 19 0
16 DRT03 G09.62+0.19 5 IR 18 06 14.4730 -20 31 31.400           ~ 2 0
17 DRT03 G09.62+0.19 6 IR 18 06 14.6470 -20 31 31.800           ~ 2 0
18 [GRM93] G09.61+0.20 E HII 18 06 14.7 -20 31 32           ~ 51 0
19 DRT03 G09.62+0.19 7 IR 18 06 14.7000 -20 31 25.100           ~ 2 0
20 [GRM93] G09.61+0.20 F Rad 18 06 14.89 -20 31 38.9           ~ 29 1
21 [GRM93] G09.61+0.20 D HII 18 06 14.9 -20 31 43           ~ 20 0
22 DPT00 G009.619+0.193 1 IR 18 06 14.9270 -20 31 40.900           ~ 2 0
23 DRT03 G09.62+0.19 9 IR 18 06 15.0930 -20 31 50.600           ~ 2 0
24 W 31 SFR 18 10 28.6 -19 55 51           ~ 280 0
25 W 31c HII 18 10 29.1 -19 56 05           ~ 357 0
26 IRAS 18097-1825A cor 18 12 39.72 -18 24 20.5           ~ 69 0
27 W 33b SFR 18 13 54.68 -18 01 48.1           ~ 85 0
28 OH 012.68-00.18 Mas 18 13 54.7457 -18 01 46.588           ~ 49 0
29 DRT03 G11.94-0.62 1 IR 18 14 00.29 -18 53 23.1           ~ 3 0
30 DRT03 G45.07+0.13 1 IR 18 14 00.29 -18 53 23.1           ~ 3 0
31 DRT03 G11.94-0.62 2 IR 18 14 00.8430 -18 53 22.800           ~ 3 0
32 DRT03 G11.94-0.62 3 IR 18 14 00.9900 -18 53 18.600           ~ 3 0
33 CORNISH G011.9368-00.6158 HII 18 14 01.0 -18 53 23           ~ 88 1
34 DRT03 G11.94-0.62 4 IR 18 14 01.0100 -18 53 25.900           ~ 3 0
35 DRT03 G11.94-0.62 5 IR 18 14 01.0500 -18 53 23.500           ~ 3 0
36 DRT03 G11.94-0.62 6 IR 18 14 01.4230 -18 53 26.900           ~ 3 0
37 DRT03 G11.94-0.62 7 IR 18 14 01.4500 -18 53 30.800           ~ 2 0
38 EGO G016.59-0.05 HII 18 21 07.9 -14 31 53           ~ 129 0
39 OH 016.59-00.05 Mas 18 21 09.0840 -14 31 48.556           ~ 85 0
40 DRT03 G19.61-0.23 1 IR 18 27 37.0800 -11 56 28.100           ~ 2 0
41 DRT03 G19.61-0.23 2 HII 18 27 37.340 -11 56 32.39           ~ 8 0
42 GAL 019.61-00.23 HII 18 27 38.0 -11 56 42           ~ 162 0
43 DRT03 G19.61-0.23 3 HII 18 27 38.14 -11 56 39.7           ~ 7 0
44 DRT03 G19.61-0.23 4 HII 18 27 38.20 -11 56 31.4           ~ 5 1
45 DRT03 G19.61-0.23 5 HII 18 27 38.79 -11 56 44.7           ~ 4 0
46 DRT03 G19.61-0.23 6 IR 18 27 38.9600 -11 56 42.700           ~ 2 0
47 GAL 028.86-00.07 HII 18 43 45.8 -03 35 30           ~ 30 0
48 IRAS 18487-0015 IR 18 51 20.6 -00 11 46           ~ 23 0
49 GAL 033.13-00.09 HII 18 52 07.96 +00 08 11.6           ~ 27 1
50 RAFGL 2271 SFR 18 53 18.54 +01 14 57.9           ~ 537 0
51 DRT03 G34.26+0.15 5 IR 18 53 18.7270 +01 15 56.700           ~ 2 0
52 GAL 035.03+00.35 cor 18 54 00.60 +02 01 19.3           ~ 48 0
53 IRAS 18538+0216 HII 18 56 22.52 +02 20 27.0           ~ 35 0
54 MSX6C G035.5789-00.0304 Y*O 18 56 22.56 +02 20 27.8           ~ 20 0
55 GAL 035.2-00.74 cor 18 58 13.00 +01 40 36.0           ~ 176 0
56 [DLW84] G35.2N HII 18 58 13.036 +01 40 36.00           ~ 138 0
57 IRAS 18556+0136 mul 18 58 13.1 +01 40 35           ~ 142 0
58 Caswell OH 035.20-01.74 Mas 19 01 45.2 +01 13 34           ~ 28 0
59 OH 035.200-01.736 Mas 19 01 45.5420 +01 13 32.690           ~ 20 0
60 [PFL97] 7 IR 19 01 45.69 +01 13 15.9           ~ 3 0
61 GAL 035.20-01.74 Y*O 19 01 46.49 +01 13 24.7           ~ 78 1
62 GAL 035.2-01.7 HII 19 01 46.50 +01 13 24.6           ~ 18 0
63 GAL 035.19-01.75 HII 19 01 47.4 +01 13 00           ~ 24 0
64 EQ 190334.9+064155 Mas 19 06 01.1 +06 46 35           ~ 18 0
65 IRAS 19035+0641 Y*O 19 06 01.6288 +06 46 36.140           ~ 84 0
66 IRAS 19095+0930 cor 19 11 54.09216 +09 35 49.6896           ~ 115 0
67 DRT03 G45.07+0.13 2 IR 19 13 22.0100 +10 50 51.600           ~ 3 0
68 IRAS 19110+1045 Y*O 19 13 22.0427 +10 50 53.336           ~ 132 0
69 DRT03 G45.07+0.13 3 IR 19 13 22.07 +10 50 55.4           ~ 3 0
70 GAL 045.47+00.13 reg 19 14 07.23 +11 12 16.6           ~ 3 1
71 RAFGL 2345 Cld 19 14 08.6 +11 12 27           ~ 64 0
72 OH 045.5+00.1 OH* 19 14 19.61808 +11 10 35.3280           O-rich 65 0
73 GAL 045.5+00.0 HII 19 14 20.8 +11 09 04           ~ 141 0
74 CORNISH G045.4545+00.0591 HII 19 14 21.31 +11 09 11.7           ~ 157 1
75 [KCW94] 048.609+00.027 Rad 19 20 30.782 +13 55 43.72           ~ 4 0
76 IRAS 19181+1349 HII 19 20 30.95 +13 55 26.7           ~ 54 0
77 [KCW94] 048.606+00.024 Rad 19 20 31.1 +13 55 23           ~ 6 0
78 NAME W 51 North Rad 19 23 40.0 +14 30 51           ~ 169 0
79 NAME W 51 IRS 1 HII 19 23 41.9 +14 30 36           ~ 124 0
80 W 51e2 Ma* 19 23 43.906 +14 30 34.48           ~ 222 0
81 W 51e4 HII 19 23 43.913 +14 30 29.49           B0.5 17 0
82 W 51e8 HII 19 23 44.2 +14 30 28           ~ 41 0
83 W 51 SNR 19 23 50 +14 06.0           ~ 1352 1
84 IRAS 20198+3716 mul 20 21 41.1 +37 25 54           ~ 17 1
85 NVSS J202141+372552 Rad 20 21 41.60 +37 25 52.1           ~ 16 2
86 GAL 075.78+00.34 cor 20 21 44.00 +37 26 38.0           ~ 131 1
87 NAME Cyg X FIR 33 Y*O 20 38 35.9 +42 37 22           B1.5 423 1
88 NAME W75N(B) cor 20 38 36.44 +42 37 34.1           ~ 52 0
89 NAME Cepheus A East SFR 22 54.3 +61 46           ~ 70 0
90 NAME Cepheus A SFR 22 56 17.9 +62 01 49           ~ 760 2
91 NAME Cep A HW 2 Y*O 22 56 17.9 +62 01 49           B0.5 243 0
92 [HW84] 4 Rad 22 56 18.5 +62 01 56           ~ 16 0
93 GAL 109.88+02.11 HII 22 56 19.4 +62 02 01           ~ 76 0

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