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BER92 - Observations of the methanol 4-1-30 E line in molecular clouds

Short title: Berulis et al. (1992)
Authors: Berulis, I. I. Kalenski, S. V. Sobolev, A. M. Streinitski, V. S.
Journal: Astronomical and Astrophysical Transactions, vol. 1, p. 231-245
Bibcode:

Non-detection table: Show non-detection table
Detection table: Show detection table (13 detection)
Target type: Class_I
Transitions: CH3OH_36(I)
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Detection table from Berulis et al. (1992)

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ID	Obs. RA	Obs. Dec	l	b	Group id	Other name	Line	V_peak	FWHM	F_peak	List	Beam	Detection	Class	Dist. (parallax)	Ref.
	(J2000)	(J2000)	(deg.)	(deg.)		Comp	CH₃OH (class I)	(km/s)	(km/s)	(Jy)		(arcsec)	Yes/No		(kpc)
1	17 47 16.8	-28 21 17.5	0.6858	-0.0091	G0.6858-0.0091		36 GHz (I);	0.421052632			AVE02	2	+CH₃OH I	SFR_MIXED		BER92
2	17 49 20.6	-27 34 8.5	1.5942	0.0063	G1.5942+0.0063		36 GHz (I);	54.2		1.27E+02	AVE02	2	+CH₃OH I	SFR		BER92
3	20 39 0.9	+42 22 37.8	81.7191	0.5695	G81.711+0.563		36 GHz (I);	0.2	0.8	1.22E+01	AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH -SiO	SFR		BER92
4	17 45 37.9	-29 05 45.7	359.8648	-0.0854	G359.8654-0.0863		36 GHz (I);	5.7	4.0	1.75E+01	AVE02	2	+H₂O +CH₃OH I +CH₃OH II	SFR_MIXED		BER92
5	19 23 42.6	+14 31 3.3	49.4944	-0.3792	G49.488-0.387		36 GHz (I);	53.0	5	8.40E+00	AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH -SiO	SFR		BER92
	19 23 42.6	+14 31 3.3	49.4944	-0.3792	G49.488-0.387		36 GHz (I);	55.3	7.0	7.80E+01	AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH -SiO	SFR		BER92
7	17 47 20.8	-28 23 17.2	0.6651	-0.0390	G0.6667-0.0344		36 GHz (I);	70.0	7	4.00E+02	AVE02	2	+H₂O +CH₃OH I +CH₃OH II -OH	SFR		BER92
8	06 41 9.8	+09 29 34.9	203.3157	2.0552	G203.316+2.055		36 GHz (I);	8.0	0.8	1.95E+04	AVE02	2	+H₂O +CH₃OH I +CH₃OH II	SFR_MIXED		BER92
9	20 38 55	+42 19 23.5	81.6651	0.5512	G81.711+0.563	West	36 GHz (I);	-2.73	0.42	3.12E+01	AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH -SiO	SFR		BER92
10	20 39 0.9	+42 21 57.9	81.7103	0.5627	G81.711+0.563		36 GHz (I);	-2.8	3.5	1.52E+01	AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH -SiO	SFR		BER92
11	02 27 3.4	+61 52 24.6	133.9465	1.0639	G133.949+1.064		36 GHz (I);	-46.2	4.4		AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		BER92
	02 27 3.4	+61 52 24.6	133.9465	1.0639	G133.949+1.064		36 GHz (I);	-48	6.0	4.80E+00	AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		BER92
13	20 39 0.9	+42 21 57.9	81.7103	0.5627	G81.711+0.563		36 GHz (I);	-5	5	1.55E+01	AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH -SiO	SFR		BER92

Distribution of sources in all sky (l,b)

Distribution of sources in all sky using Aladin

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Distribution of sources in IRAS color-color diagram

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Original color diagram is taken form van der Veen & Habing (1987)

Type	Description
I	Oxygen-rich non-variable stars without circumstellar shells
II	Variable stars with "young" O-rich circumstellar shells
IIIa	Variable stars with more evolved O-rich circumstellar shells
IIIb	Variable stars with thick O-rich circumstellar shells
IV	Variable stars with very thick O-rich circumstellar shells
V	Planetary nebulae and non- variable stars with very cool circumstellar shells
VIa	Variable stars with relatively cold dust at large distances; a significant part of the stars is carbon-rich
VIb	Variable stars with relatively hot dust close to the star and relatively cold dust at large distances; Some of the objects have proven to be O-rich
VII	Variable stars with more evolved C-rich circumstellar shells
VIII	Different sort of objects

Distribution of the detection velocities versus galactic longitude from BER92

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