Display data from paper

Select data type:

KAL92 - A search for methanol masers at 44 GHz

Short title: Kalenskij et al. (1992)
Authors: Kalenskij, S. V. Bachiller, R. Berulis, I. I. Val'tts, I. E. Gomez-Gonzalez, J. Martin-Pintado, J. Rodriguez-Franco, A. Slysh, V. I.
Journal: Astronomicheskij Zhurnal (ISSN 0004-6299), vol. 69, no. 5, p. 1002-1014.
Bibcode:

Target type: YSO,IRAS

Abstract
Results of an extensive survey of young stellar objects in the methanol line 7(0) - 6(1)A(+) (44 GHz) are presented. Three new masers were detected towards cold IRAS sources in the dark clouds L 291 (GGD 27), L 379, and IC 1396 N. The new masers were also observed in 4(-1) - 3(0) E (36 GHz) and 1(0) - 0(0)A(+) (48 GHz) methanol transitions. A relationship between methanol masers and high-velocity flows with dense disks around central sources is proposed, and a possible correlation between maser emission and their intensity in the FIR is suggested.

Abstract

Results of an extensive survey of young stellar objects in the methanol line 7(0) - 6(1)A(+) (44 GHz) are presented. Three new masers were detected towards cold IRAS sources in the dark clouds L 291 (GGD 27), L 379, and IC 1396 N. The new masers were also observed in 4(-1) - 3(0) E (36 GHz) and 1(0) - 0(0)A(+) (48 GHz) methanol transitions. A relationship between methanol masers and high-velocity flows with dense disks around central sources is proposed, and a possible correlation between maser emission and their intensity in the FIR is suggested.

Download as: Table (CSV)
View as list of objects

Detection table from Kalenskij et al. (1992)

Export table to csv

Hide / Show individual components

ID	Obs. RA	Obs. Dec	l	b	Group id	Line	V_peak	FWHM	F_peak	List	Beam	Detection	Class	Dist. (parallax)	Ref.
	(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	36 GHz (I);	14		1.70E+01	AVE02	2	+H₂O +CH₃OH I -CH₃OH II	SFR_MIXED		KAL92
2	18 19 12.9	-20 47 13.6	10.8471	-2.5921	G10.841-2.592	44 GHz (I);	13.5	0.8	1.35E+02	AVE02	2	+H₂O +CH₃OH I -CH₃OH II	SFR_MIXED		KAL92
3	18 29 24.8	-15 15 48.9	16.8683	-2.1582	G16.868-2.158	44 GHz (I);	18.0	1.1	1.08E+02	AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		KAL92
	18 29 24.8	-15 15 48.9	16.8683	-2.1582	G16.868-2.158	44 GHz (I);	19.0	3.3	1.08E+02	AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		KAL92
5	18 29 24.8	-15 15 48.9	16.8683	-2.1582	G16.868-2.158	36 GHz (I);	18.0	1.9	7.40E+01	AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		KAL92
	18 29 24.8	-15 15 48.9	16.8683	-2.1582	G16.868-2.158	36 GHz (I);	20.4	1.2	7.40E+01	AVE02	2	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		KAL92
7	21 40 42.4	+58 16 9.7	99.9825	4.1696	G99.982+4.170	44 GHz (I);	-0.5	0.6	1.50E+01	AVE02	2	+H₂O +CH₃OH I -CH₃OH II +OH	GALAXY		KAL92

DSS colored	2MASS colored	WISE colored
PACS color (70-160 um)	SPIRE color (250-500 um)	GLIMPSE 360
SDSS color	IRAC color I1,I2,I4	NVSS (1.4GHz)
ATLASGAL 870 um	ATLASGAL 870 um + Planck	Bolocam 1.1 mm
UKIDSS K Download UKIDSS K FITS	2MASS K Download 2MASS K FITS

select MAX(met1_data_all.ra_hms) as ra_hms,MAX(met1_data_all.dec_dms) as dec_dms,MAX(met1_data_all.source_name) as source_name,MAX(met1_data_all.ra) as ra,MAX(met1_data_all.dec) as dec,MAX(met1_data_all.l) as l,MAX(met1_data_all.b) as b,MAX(met1_data_all.grp) as grp,MAX(met1_data_all.other_name) as other_name,MAX(met1_data_all.other_desc) as other_desc,BOOL_OR(thermal) as thermal,MAX(met1_data_all.line) as line,MAX(met1_data_all.vrange) as vrange,MAX(met1_data_all.vpeak) as vpeak,MAX(met1_data_all.peak) as peak,MAX(met1_data_all.fwhm) as fwhm,MAX(met1_data_all.int) as int,MAX(met1_data_all.rms) as rms,MAX(met1_data_all.units) as units,MAX(met1_data_all.units_rms) as units_rms,MAX(met1_data_all.date_txt) as date_txt,MAX(met1_data_all.telescope_ref) as telescope_ref,MAX(met1_data_all.telescope_conf) as telescope_conf,MAX(met1_data_all.v_step) as v_step,MAX(met1_data_all.beam) as beam,MAX(met1_data_all.beam_maj) as beam_maj,MAX(met1_data_all.beam_min) as beam_min,MAX(met1_data_all.beam_pa) as beam_pa,MAX(met1_data_all.ref) as ref,MAX(met1_data_all.list_ref) as list_ref,MAX(met1_data_all.ascii) as ascii,MAX(met1_data_all.url) as url,MAX(met1_data_all.image) as image,MAX(met1_data_all.image2) as image2,MAX(met1_data_all.image3) as image3,MAX(met1_data_all.descr) as descr,MAX(met1_data_all.id) as id,BOOL_OR(mjy_flag) as mjy_flag,BOOL_OR(rms_mjy_flag) as rms_mjy_flag,MAX(met1_data_all.dist) as dist,1 as dist_parallax,MAX(met1_data_all.date_txt) as date_txt,MAX(line_det) as line_det,MAX(type) as type,MAX(simbad_types_cat) as simbad_types_cat FROM met1_data_all  LEFT JOIN all_objects_withmet ON met1_data_all.grp=all_objects_withmet.group_name LEFT JOIN object_categories ON all_objects_withmet.group_name = object_categories.group_name_cat AND object_categories.tbl_cat = 'all_objects_withmet' LEFT JOIN transitions ON met1_data_all.line=transitions."Line"  WHERE ref ilike 'KAL92' AND detected=true AND hide=false GROUP BY ref

select met1_data_all.ra_hms,met1_data_all.dec_dms,met1_data_all.source_name,met1_data_all.ra,met1_data_all.dec,met1_data_all.l,met1_data_all.b,met1_data_all.grp,met1_data_all.other_name,met1_data_all.other_desc,met1_data_all.thermal,met1_data_all.line,met1_data_all.vrange,met1_data_all.vpeak,met1_data_all.peak,met1_data_all.fwhm,met1_data_all.int,met1_data_all.rms,met1_data_all.units,met1_data_all.units_rms,met1_data_all.date_txt,met1_data_all.telescope_ref,met1_data_all.telescope_conf,met1_data_all.v_step,met1_data_all.beam,met1_data_all.beam_maj,met1_data_all.beam_min,met1_data_all.beam_pa,met1_data_all.ref,met1_data_all.list_ref,met1_data_all.ascii,met1_data_all.url,met1_data_all.image,met1_data_all.image2,met1_data_all.image3,met1_data_all.descr,met1_data_all.id,met1_data_all.mjy_flag,met1_data_all.rms_mjy_flag,met1_data_all.dist,met1_data_all.dist_parallax,met1_data_all.date_txt,line_det,type,simbad_types_cat FROM met1_data_all   LEFT JOIN all_objects_withmet ON met1_data_all.grp=all_objects_withmet.group_name LEFT JOIN object_categories ON all_objects_withmet.group_name = object_categories.group_name_cat AND object_categories.tbl_cat = 'all_objects_withmet' LEFT JOIN transitions ON met1_data_all.line=transitions."Line"  WHERE ref ilike 'KAL92' AND detected=true AND hide=false ORDER BY detected DESC,id

Display data from paper

KAL92 - A search for methanol masers at 44 GHz

View as list of objects

Detection table from Kalenskij et al. (1992)