1995A&A...294..825V


C.D.S. - SIMBAD4 rel 1.7 - 2020.12.02CET20:40:25

1995A&A...294..825V - Astronomy and Astrophysics, volume 294, 825-830 (1995/2-3)

The discovery of methanol masers at 107 GHz.

VAL'TTS I.E., DZURA A.M., KALENSKII S.V., SLYSH V.I., BOOTH R.S. and WINNBERG A.

Abstract (from CDS):

A new methanol maser line at 107GHz was discovered in five galactic sources. All of them are known Class II methanol masers. Toward Class I methanol maser sources, the 107-GHz line was found in absorption, or as rather weak quasi-thermal emission sources. The detection of these new methanol masers supports an assumption that the level population inversion is due to overpopulation of some K ladders relative to neighbouring ladders.

Abstract Copyright:

Journal keyword(s): line: profiles - masers - molecular processes - ISM: molecules - radio lines: ISM

Simbad objects: 50

goto View the reference in ADS

Number of rows : 50

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 IC 1795 HII 02 25 43.5 +62 06 13           ~ 229 0
2 NAME W 3 OH HII 02 27 04.1 +61 52 22           ~ 947 2
3 W 3 MoC 02 27 04.10 +61 52 27.1           ~ 969 3
4 NAME Ori-S6 PoC 05 35 12.7 -05 24 08           ~ 37 0
5 NAME Orion-KL SFR 05 35 14.16 -05 22 21.5           ~ 2032 1
6 OMC 2 MoC 05 35 27 -05 10.1           ~ 394 1
7 SH 2-231 HII 05 39 12.9 +35 45 54           ~ 121 0
8 [M91] B053606.4+352921 Mas 05 39 27.6 +35 30 58           ~ 8 0
9 NAME Mon R2 HII 06 07 46.6 -06 22 59           ~ 659 2
10 SH 2-252 A HII 06 08 33 +20 39.3           ~ 73 0
11 NGC 2175 OpC 06 09 39 +20 29.2   7.0 6.8     ~ 248 3
12 NAME SH 2-255 IRS 1 Y*O 06 12 54.0060 +17 59 22.958           ~ 321 0
13 IC 2162 HII 06 13 04.1 +17 58 44           ~ 339 2
14 LBN 196.49-01.60 HII 06 14 38.40 +13 49 44.7           ~ 162 1
15 NGC 2264 OpC 06 40 58 +09 53.7     3.9     ~ 1606 1
16 Caswell OH 232.621+00.996 Mas 07 32 10.0 -16 58 15           ~ 7 0
17 LBN 37 HII 15 59.9 -01 36           ~ 4 0
18 NAME Sgr B2 MoC 17 47 20.4 -28 23 07           ~ 1956 1
19 GAL 009.62+00.19 HII 18 06 13.9 -20 31 44           ~ 188 0
20 GAL 008.67-00.30 HII 18 06 19.027 -21 37 32.32           ~ 64 0
21 W 31 SFR 18 10 28.6 -19 55 51           ~ 241 0
22 W 33a Y*O 18 14 39.0 -17 52 03           ~ 590 0
23 [M91] B182455.8-111624 Mas 18 27 44.1 -11 14 54           ~ 12 0
24 [SKV94] 023.01-0.41 Mas 18 34 40.94 -09 00 52.8           ~ 8 0
25 GRS G024.80 +00.10 SFR 18 38 14.8 -06 47 39           ~ 102 0
26 SRBY 162 Mas 18 46 03.6 -02 39 26           ~ 31 1
27 Caswell OH 030.82+00.28 Mas 18 46 36.3 -01 45 12           ~ 7 0
28 [VES2000] 184458.90-020427.0 Mas 18 47 34.96 -02 01 06.0           ~ 8 0
29 GAL 035.2-00.74 MoC 18 58 13 +01 40.6           ~ 154 0
30 OH 35.19 -0.74 Mas 18 58 13.02 +01 40 35.2           ~ 36 0
31 IRAS 18556+0136 mul 18 58 13.1 +01 40 35           ~ 133 0
32 SNR G035.2-01.8 SNR 19 01.6 +01 14           ~ 145 0
33 [SHK2000] 19095+0930 Mas 19 11 53.5230 +09 35 53.621           ~ 32 0
34 [MWH86] W 51 Met 5 Mas 19 23 38.2 +14 30 05           ~ 8 0
35 [MWH86] W 51 Met 4 Mas 19 23 43.2 +14 31 34           ~ 7 0
36 [MWH86] W 51 Met 1 Mas 19 23 43.9 +14 29 25           ~ 8 0
37 [MWH86] W 51 Met 3 Mas 19 23 45.2 +14 29 45           ~ 11 0
38 [VES2000] 192128.90+142348.0 Mas 19 23 46.5 +14 29 41           ~ 12 0
39 W 51 SNR 19 23 50 +14 06.0           ~ 1160 1
40 NAME DR 21(OH) M Rad 20 39 01 +42 29.8           ~ 84 0
41 W 75(OH) Rad 20 39 01.01 +42 22 49.9           ~ 37 0
42 [MBS2007c] CygX-N44 Rad 20 39 01.01 +42 22 50.2           ~ 363 0
43 GRS G081.70 +00.50 SFR 20 39 01.6 +42 19 38           O4.5 952 0
44 NGC 7000 HII 20 58 47 +44 19.8           ~ 365 1
45 IC 1396 OpC 21 39 00 +57 29.4           ~ 447 1
46 SH 2-140 OpC 22 19 07.8 +63 17 07           ~ 635 2
47 IRAS 22176+6303 Y*O 22 19 17.978 +63 18 52.92           ~ 590 0
48 NAME Cepheus A SFR 22 56 17.9 +62 01 49           ~ 702 2
49 NGC 7538 OpC 23 13 37 +61 30.0           ~ 831 0
50 NGC 7538S Y*O 23 13 44.8 +61 26 51           ~ 73 1

    Equat.    Gal    SGal    Ecl

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2020.12.02-20:40:25

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