Display data from paper

Select data type:

KAL93 - A study of methanol masers at 36 and 44 GHz and 48 GHz thermal emission around them

Short title: Kalenskij et al. (1993)
Authors: Kalenskij, S. V. Berulis, I. I. Val'tts, I. E. Slysh, V. I. Bachiller, R. Gomez-Gonzalez, J. Martin-Pintado, J. Rodriguez-Franco, A.
Journal: In: Astrophysical masers; Proceedings of the Conference, Arlington, VA, Mar. 9-11, 1992 (A93-52776 23-90), p. 191-194.
Bibcode:

Non-detection table: Show non-detection table
Detection table: Show detection table (7 detection) Non-detection table: Show non-detection table (1 non-detection)
Target type: IRAS
Transitions: CH3OH_36(I),CH3OH_44(I)

Abstract
An extensive search for new methanol sources were made. Three new masers in the 7(0)-6(1) A(+) transition and twenty-four new thermal sources in the 1(0)-0(0)A(+) transition were detected. Our results support the idea that high-velocity flows may increase the abundance of methanol and that methanol masers arise in methanol-rich sources.

Download as: Table (CSV)
View paper data

Detection table from Kalenskij et al. (1993)

Export table to csv

Hide / Show individual components

ID	Obs. RA	Obs. Dec	l	b	Group id	Source name	Line	V_peak	FWHM	F_peak	Beam	Detection	Class	Dist. (parallax)
	(J2000)	(J2000)	(deg.)	(deg.)			CH₃OH (class I)	(km/s)	(km/s)	(Jy)	(arcsec)	Yes/No		(kpc)
1	18 19 12.9	-20 47 13.6	10.8471	-2.5921	G10.841-2.592	GGD 27	44 GHz (I);	13.5	0.8	135	120	+H₂O +CH₃OH I +CH₃OH II	SFR_MIXED
2	18 19 12.9	-20 47 13.6	10.8471	-2.5921	G10.841-2.592	GGD 27	36 GHz (I);	14	<1	17	120	+H₂O +CH₃OH I +CH₃OH II	SFR_MIXED
3	18 29 24.8	-15 15 48.9	16.8683	-2.1582	G16.868-2.158	L 379	44 GHz (I);	18	1.1	63	120	+H₂O +CH₃OH I +CH₃OH II	SFR
	18 29 24.8	-15 15 48.9	16.8683	-2.1582	G16.868-2.158	L 379	44 GHz (I);	19	3.3	45	120	+H₂O +CH₃OH I +CH₃OH II	SFR
5	18 29 24.8	-15 15 48.9	16.8683	-2.1582	G16.868-2.158	L 379	36 GHz (I);	18	1.9	36	120	+H₂O +CH₃OH I +CH₃OH II	SFR
	18 29 24.8	-15 15 48.9	16.8683	-2.1582	G16.868-2.158	L 379	36 GHz (I);	20.4	1.2	38	120	+H₂O +CH₃OH I +CH₃OH II	SFR
7	21 40 42.4	+58 16 9.7	99.9825	4.1696	G99.982+4.170	IC 1396N	44 GHz (I);	-0.5	0.6	15	120	+H₂O +CH₃OH I +CH₃OH II	GALAXY

Non-detection table from Kalenskij et al. (1993)

Export table to csv

Hide / Show individual components

ID	Obs. RA	Obs. Dec	l	b	Group id	Source name	Line	F_peak	Beam	Detection	Class
	(J2000)	(J2000)	(deg.)	(deg.)			CH₃OH (class I)	(Jy)	(arcsec)	Yes/No
1	21 40 42.4	+58 16 9.7	99.9825	4.1696	G99.982+4.170	IC 1396N	36 GHz (I);	<6	120	+H₂O +CH₃OH I +CH₃OH II	GALAXY

Distribution of sources in all sky (l,b)

Distribution of sources in all sky using Aladin

Tip: Click on some source to get more informaiton

Distribution of sources in IRAS color-color diagram

Tip: Use "Box select" or "Lasso select" to display colour-selected sources in Aladin all-sky view

Tip: Click on some source to look at the different surveys. You must select some surveys in previous page at "View images"

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 KAL93

Tip: Use "Box select" or "Lasso select" to display velocity-selected sources in Aladin all-sky view