CDS

2000A&AS..147..181S

Query : 2000A&AS..147..181S

2000A&AS..147..181S - Astron. Astrophys., Suppl. Ser., 147, 181-185 (2000/December-1)

New detections of OH sources towards the 6.7 GHz methanol masers.

SZYMCZAK M. and KUS A.J.

Abstract (from CDS):

A sample of 6.7GHz methanol masers has been searched for OH maser emission at 1665 and 1667 MHz using the 32 m Torun radio telescope. Eight new OH sources were detected. They are generally weak at radio and infrared wavelengths. In the northern hemisphere sample of 68 methanol sources the OH maser emission is associated with 49 sources. Generally OH masers do not arise in weak FIR sources. The ratio of OH to CH3OH maser flux densities increases for objects with blue FIR colour and probably reflects evolutionary changes in the star-forming regions.

Abstract Copyright: ∼

Journal keyword(s): masers - surveys - stars: formation - ISM: molecules - radio lines: ISM - HII regions

CDS comments: Masers in Table 1 = [SHK2000] HHMMm+DDMM.

Simbad objects: 35

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Number of rows : 35
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023 		#notes
1 IRAS 02455+6034 HII 02 49 23.2 +60 47 01           ~ 19 0
2 [SHK2000] 05382+3547 Mas 05 41.6 +35 48           ~ 2 0
3 RAFGL 5165 IR 05 41 37.4 +35 48 49           ~ 19 0
4 IRAS 06061+2151 SFR 06 09 07.8 +21 50 39           ~ 82 0
5 IRAS 18494+0002 MIR 18 51 59.40216 +00 06 33.8256           ~ 3 0
6 [BK2004] J185328.7+003158 Mas 18 53 28.7 +00 31 58           ~ 15 0
7 IRAS 18512+0029 * 18 53 45.9767730168 +00 33 33.068863224           ~ 6 0
8 [ERG2015] 6375 smm 18 55 16.5 +03 05 07           ~ 25 0
9 IRAS 18572+0057 HII 18 59 49.0 +01 01 34           ~ 11 0
10 GAL 037.55-00.11 HII 19 00 15.7 +04 03 13           ~ 40 0
11 IRAS 19012+0505 mul 19 03 43.5 +05 09 49           ~ 30 0
12 [CPA2006] N75 bub 19 03 47.1 +05 09 27           ~ 40 0
13 TYC 474-681-1 * 19 05 36.4468168152 +06 25 59.577312720   11.76 11.41 11.58   ~ 7 0
14 IRAS 19048+0705 FIR 19 07 16.9 +07 10 02           ~ 5 0
15 GAL 043.18-00.52 HII 19 12 23.19 +08 32 12.2           ~ 37 0
16 GAL 043.89-00.78 HII 19 14 26.16 +09 22 34.0           ~ 51 0
17 IRAS 19186+1440 IR 19 20 57.0 +14 46 40           ~ 10 0
18 IRAS 19189+1520 IR 19 21 11.5 +15 25 59           ~ 4 0
19 [SHK2000] 19191+1538 Mas 19 21.4 +15 44           ~ 2 0
20 IRAS 19191+1538 HII 19 21 27.2 +15 44 15           ~ 14 0
21 AGAL G053.037+00.112 cor 19 28 55.5 +17 52 00           ~ 45 0
22 MSX6C G053.1417+00.0705 Y*O 19 29 17.556 +17 56 20.62           ~ 13 0
23 [SHK2000] 19282+1814 Mas 19 30.4 +18 20           ~ 2 0
24 IRAS 19282+1814 HII 19 30 28.1 +18 20 53           ~ 36 0
25 [SHK2000] 19366+2301 Mas 19 38.7 +23 08           ~ 2 0
26 BLAST J193849+230839 HII 19 38 47.10 +23 08 28.1           ~ 17 1
27 IRAS 19388+2357 Y*O 19 40 59.1 +24 04 46           ~ 28 0
28 [SHK2000] 20062+3550 Mas 20 08.1 +35 59           ~ 2 0
29 IRAS 20062+3550 HII 20 08 09.8 +35 59 20           ~ 20 0
30 [SHK2000] 21074+4949 Mas 21 09.1 +50 01           ~ 2 0
31 IRAS 21074+4949 IR 21 09 08.1 +50 02 00           ~ 11 0
32 [MSS98] 23 Mas 22 28.9 +64 13           ~ 3 0
33 NAME SH 2-152 SE * 22 58 42.6 +58 47 45           ~ 50 1
34 IRAS 23139+5939 Y*O 23 16 10.3420 +59 55 28.596           ~ 91 0
35 IRAS 18049+0712 IR ~ ~           ~ 1 0

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2023.04.01-17:06:58

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