Display data from paper

Select data type: ,

COD00 - On the occurrence of the 6.7 GHz CH₃OH maser emission in UCH bt II regions

Short title: Codella & Moscadelli (2000)
Authors: Codella, C.Moscadelli, L.
Journal: Astronomy and Astrophysics, v.362, p.723-729 (2000)
Bibcode:

Target type: UCHII
Transitions: CH3OH_6(II)

Abstract
We present the results of a statistical survey of the 6.7 GHz CH₃OH and 22.2 GHz H₂O emissions towards a large homogeneous sample of ultracompact (UC) H II regions, performed to investigate the nature of the methanol emission: does it point out ionized regions or does it trace earlier stages of the star forming process? The present detection rates are almost identical: 23% for CH₃OH and 22% for H_2O. Even considered the uncertainties of the survey, the large number of non-detections is consistent with the scenario where methanol masers disappear during the UC phase, like water masers do. Moreover, the probability to have the CH₃OH counterpart of a H₂O source is at least 40%, indicating that these maser emissions are emphasizing two at least partly overlapping evolutionary phases. The comparison between the velocity ranges suggests that methanol and water masers form in different gas components related to the star forming process.

Abstract

We present the results of a statistical survey of the 6.7 GHz CH₃OH and 22.2 GHz H₂O emissions towards a large homogeneous sample of ultracompact (UC) H II regions, performed to investigate the nature of the methanol emission: does it point out ionized regions or does it trace earlier stages of the star forming process? The present detection rates are almost identical: 23% for CH₃OH and 22% for H_2O. Even considered the uncertainties of the survey, the large number of non-detections is consistent with the scenario where methanol masers disappear during the UC phase, like water masers do. Moreover, the probability to have the CH₃OH counterpart of a H₂O source is at least 40%, indicating that these maser emissions are emphasizing two at least partly overlapping evolutionary phases. The comparison between the velocity ranges suggests that methanol and water masers form in different gas components related to the star forming process.

Download as: Table (CSV)
View paper statistics

Detection table from Codella & Moscadelli (2000)

Export table to csv

Hide / Show individual components

ID	Obs. RA	Obs. Dec	l	b	Group id	Source name	Image	V_range	V_peak	FWHM	F_peak	∫F dv	Telescope	RMS	Beam	Detection	Date
	(J2000)	(J2000)	(deg.)	(deg.)				(km/s)	(km/s)	(km/s)	(Jy)	(Jy*km/s)		(Jy)	(arcsec)	Yes/No
1	18 33 23.8	-08 33 33.7	23.2650	0.0770	G23.265+0.078	23.265+0.077	Image	76.2;82.4	+0.077	0.65 (0.05)	10.6 (1.2)	16.8 (2.0)	MED	1.400	114	+H₂O +CH₃OH I -CH₃OH II +OH	1993-1994
2	19 10 33.4	+09 08 24.8	43.2370	-0.0450	G43.237-0.046	43.237-0.045	Image	-119.9;23.0	-0.045	0.75 (0.33)	132.0 (4.7)	711.7 (12.9)	MED	1.300	114	+H₂O +CH₃OH I -CH₃OH II	1993-1994

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

select MAX(h2o_data_all.ra_hms) as ra_hms,MAX(h2o_data_all.dec_dms) as dec_dms,MAX(h2o_data_all.source_name) as source_name,MAX(h2o_data_all.ra) as ra,MAX(h2o_data_all.dec) as dec,MAX(h2o_data_all.l) as l,MAX(h2o_data_all.b) as b,MAX(h2o_data_all.grp) as grp,MAX(h2o_data_all.other_name) as other_name,MAX(h2o_data_all.other_desc) as other_desc,BOOL_OR(thermal) as thermal,MAX(h2o_data_all.vrange) as vrange,MAX(h2o_data_all.vpeak) as vpeak,MAX(h2o_data_all.peak) as peak,MAX(h2o_data_all.fwhm) as fwhm,MAX(h2o_data_all.int) as int,MAX(h2o_data_all.rms) as rms,MAX(h2o_data_all.units) as units,MAX(h2o_data_all.units_rms) as units_rms,MAX(h2o_data_all.date_txt) as date_txt,MAX(h2o_data_all.telescope_ref) as telescope_ref,MAX(h2o_data_all.beam) as beam,MAX(h2o_data_all.beam_maj) as beam_maj,MAX(h2o_data_all.beam_min) as beam_min,MAX(h2o_data_all.beam_pa) as beam_pa,MAX(h2o_data_all.ref) as ref,MAX(h2o_data_all.list_ref) as list_ref,MAX(h2o_data_all.ascii) as ascii,MAX(h2o_data_all.image) as image,MAX(h2o_data_all.descr) as descr,MAX(h2o_data_all.id) as id,BOOL_OR(mjy_flag) as mjy_flag,BOOL_OR(rms_mjy_flag) as rms_mjy_flag,MAX(h2o_data_all.dist) as dist,MAX(h2o_data_all.date_txt) as date_txt,MAX(line_det) as line_det FROM h2o_data_all  LEFT JOIN all_objects_withmet ON h2o_data_all.grp=all_objects_withmet.group_name  WHERE ref ilike 'COD00' AND detected=true AND hide=false GROUP BY ref

select h2o_data_all.ra_hms,h2o_data_all.dec_dms,h2o_data_all.source_name,h2o_data_all.ra,h2o_data_all.dec,h2o_data_all.l,h2o_data_all.b,h2o_data_all.grp,h2o_data_all.other_name,h2o_data_all.other_desc,h2o_data_all.thermal,h2o_data_all.vrange,h2o_data_all.vpeak,h2o_data_all.peak,h2o_data_all.fwhm,h2o_data_all.int,h2o_data_all.rms,h2o_data_all.units,h2o_data_all.units_rms,h2o_data_all.date_txt,h2o_data_all.telescope_ref,h2o_data_all.beam,h2o_data_all.beam_maj,h2o_data_all.beam_min,h2o_data_all.beam_pa,h2o_data_all.ref,h2o_data_all.list_ref,h2o_data_all.ascii,h2o_data_all.image,h2o_data_all.descr,h2o_data_all.id,h2o_data_all.mjy_flag,h2o_data_all.rms_mjy_flag,h2o_data_all.dist,h2o_data_all.date_txt,line_det FROM h2o_data_all   LEFT JOIN all_objects_withmet ON h2o_data_all.grp=all_objects_withmet.group_name  WHERE ref ilike 'COD00' AND detected=true AND hide=false ORDER BY detected DESC,id

Display data from paper

COD00 - On the occurrence of the 6.7 GHz CH3OH maser emission in UCH bt II regions

View paper statistics

Detection table from Codella & Moscadelli (2000)

COD00 - On the occurrence of the 6.7 GHz CH₃OH maser emission in UCH bt II regions