1998AJ....116.1897M


Query : 1998AJ....116.1897M

1998AJ....116.1897M - Astron. J., 116, 1897-1905 (1998/October-0)

Masers in massive star-forming regions associated with the brightest steep-spectrum IRAS point sources.

MacLEOD G.C., SCALISE E.Jr, SAEDT S., GALT J.A. and GAYLARD M.J.

Abstract (from CDS):

Twenty-four bright, steep-spectrum far-infrared IRAS point sources, which were originally discussed by Hughes & MacLeod, have been searched for hydroxyl, water, and methanol masers and for formaldehyde absorption features. Distances and spectral types for the stars exciting these masers were estimated using radio continuum, IRAS spectra, and maser velocity data. It is found that 21 of the 24 sources are regions of massive star formation containing stars earlier than type B2. We report the discovery of five new OH masers, one new 6.7 GHz CH3OH maser, and two new 12.2 GHz CH3OH masers toward these IRAS sources. By contrast, no 4.765 GHz excited-OH masers were found toward these sources. This sample contains only star-forming regions; there are no planetary or reflection nebulae or extragalactic sources present, as seen in samples with less extreme IRAS colors.

Abstract Copyright: ∼

Journal keyword(s): ISM: H II Regions - ISM: Masers - Stars: Formation

Nomenclature: Table 2: [MSS98] NN (Nos 1-24).

Simbad objects: 47

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Number of rows : 47
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 [MSS98] 1 Mas 05 51.1 +25 46           ~ 1 0
2 IRAS 05480+2545 HII 05 51 10.8 +25 46 14           ~ 34 0
3 GAL 192.16-03.82 HII 05 58 13.4 +16 32 00           ~ 145 1
4 [PBC91] B055520.3+163146 Mas 05 58 13.9 +16 32 00           ~ 4 0
5 IRAS 07427-2400 HII 07 44 51.997 -24 07 42.11           ~ 78 0
6 IRAS 12091-6129 of? 12 11 47.65 -61 46 20.9           ~ 27 0
7 OH 301.14-00.23 Mas 12 35 35.14 -63 02 32.6           ~ 22 0
8 IRAS 12326-6245 HII 12 35 35.184 -63 02 29.40           ~ 55 0
9 IRAS 14498-5856 HII 14 53 42.324 -59 08 57.44           ~ 38 0
10 OH 318.05+00.08 Mas 14 53 42.67 -59 08 52.4           ~ 16 0
11 [MSS98] 7 Mas 15 39.9 -56 04           ~ 1 0
12 IRAS 15360-5554 HII 15 39 56.2 -56 04 00           ~ 13 0
13 [MSS98] 8 Mas 15 55.8 -52 43           ~ 1 0
14 IRAS 15520-5234 HII 15 55 48.336 -52 43 10.20           ~ 59 1
15 [MSS98] 9 Mas 16 09.8 -51 54           ~ 1 0
16 IRAS 16060-5146 HII 16 09 52.776 -51 54 52.20           ~ 44 0
17 OH 340.24-00.06 Mas 16 48 05.18 -45 05 08.4           ~ 9 0
18 IRAS 16445-4459 HII 16 48 05.2 -45 05 09           ~ 39 0
19 IRAS 16547-4247 Y*O 16 58 17.208 -42 52 08.16           ~ 187 0
20 OH 344.58-00.02 Y*? 17 02 57.71 -41 41 53.8           ~ 43 0
21 IRAS 16596-4012 HII 17 03 06.4 -40 17 09           ~ 9 0
22 OH 345.00-00.22 Mas 17 05 09.5 -41 29 04           ~ 34 0
23 IRAS 17016-4124 SFR 17 05 11.160 -41 29 06.00           ~ 75 0
24 OH 351.75-00.53 Mas 17 26 42.57 -36 09 17.6           ~ 74 1
25 IRAS 17233-3606 HII 17 26 42.8 -36 09 17           ~ 98 0
26 [MSS98] 16 Mas 17 38.5 -31 55           ~ 1 0
27 IRAS 17352-3153 HII 17 38 30.6 -31 54 41           ~ 8 0
28 [MSS98] 17 Mas 18 29.4 -15 15           ~ 1 0
29 IRAS 18265-1517 out 18 29 24.8 -15 15 49           ~ 67 0
30 EQ 190334.9+064155 Mas 19 06 01.1 +06 46 35           ~ 18 0
31 IRAS 19035+0641 Y*O 19 06 01.6288 +06 46 36.140           ~ 84 0
32 [PBC91] B190852.3+090225 Mas 19 11 15.8 +09 07 27           ~ 4 0
33 IRAS 19088+0902 Rad 19 11 15.9 +09 07 27           ~ 22 0
34 OH 043.796-00.127 Mas 19 11 53.9868 +09 35 50.325           ~ 89 0
35 IRAS 19095+0930 cor 19 11 54.09216 +09 35 49.6896           ~ 115 0
36 [KCW94] 069.540-00.975 HII 20 10 08.95 +31 31 35.4           ~ 168 1
37 IRAS 20081+3122 Y*O 20 10 09.036 +31 31 34.14           ~ 172 0
38 Onsala 1 cor 20 10 09.2036 +31 31 36.090           ~ 194 0
39 IRAS 20126+4104 Y*O 20 14 25.8816769656 +41 13 36.879427236           B2.5-B0.5 469 0
40 [MSS98] 13 Mas 21 02.8 -40 00           ~ 1 0
41 LDN 1206 DNe 22 28 52.2 +64 13 43           ~ 70 0
42 IRAS 22272+6358A Cld 22 28 52.2 +64 13 43           ~ 53 0
43 [MSS98] 23 Mas 22 28.9 +64 13           ~ 3 0
44 NAME Cepheus A SFR 22 56 17.9 +62 01 49           ~ 760 2
45 GAL 109.87+02.11 Mas 22 56 18.1 +62 01 46           ~ 12 0
46 GAL 109.88+02.11 HII 22 56 19.4 +62 02 01           ~ 76 0
47 Caswell OH 240.16+00.071 Mas ~ ~           ~ 1 0

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