Display data from paper

Select data type:

CER90 - Detection of 183 GHz water vapour maser emission from interstellar andcircumstellar sources.

Short title: Cernicharo et al. (1990)
Authors: Cernicharo, J.Thum, C.Hein, H.John, D.Garcia, P.Mattioco, F.
Journal: Astronomy and Astrophysics, Vol. 231, p. L15-L18 (1990)
Bibcode:

Target type: Low_mass_SFR,star
Transitions: H2O_183

Abstract
The IRAM 30-m telescope was used to observe the emission of the 183 GHz 3(13)-2(20) rotational transition of water from a selected sample of giant molecular clouds, low mass star forming regions and evolved stars. The zenith atmospheric transmission was 25-30 percent during the observations. The water emission shows strong and narrow masing lines (flux = about 1000-15000 Jy) toward the hot molecular clouds with strong 22 GHz water masers. Broad line emission, perhaps of thermal origin, is found in the sources associated with molecular outflows. Double peaked profiles, corresponding to masing lines (flux = about 100-600 Jy), are observed toward the evolved stars. Finally, 183 GHz maser emission is also observed in the more quiescent clouds, but at velocities different from those of the associated 22 GHz masers.

Abstract

The IRAM 30-m telescope was used to observe the emission of the 183 GHz 3(13)-2(20) rotational transition of water from a selected sample of giant molecular clouds, low mass star forming regions and evolved stars. The zenith atmospheric transmission was 25-30 percent during the observations. The water emission shows strong and narrow masing lines (flux = about 1000-15000 Jy) toward the hot molecular clouds with strong 22 GHz water masers. Broad line emission, perhaps of thermal origin, is found in the sources associated with molecular outflows. Double peaked profiles, corresponding to masing lines (flux = about 100-600 Jy), are observed toward the evolved stars. Finally, 183 GHz maser emission is also observed in the more quiescent clouds, but at velocities different from those of the associated 22 GHz masers.

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

Detection table from Cernicharo et al. (1990)

Export table to csv

Hide / Show individual components

ID	Obs. RA	Obs. Dec	l	b	Group id	Source name	Image	Line	V_peak	T_a	∫T_a dv	Telescope	Beam	Detection	Class	Dist. (parallax)	Date
	(J2000)	(J2000)	(deg.)	(deg.)				H₂O	(km/s)	(K)	(K*km/s)		(arcsec)	Yes/No		(kpc)
1	22 56 18.1	+62 01 46.3	109.8708	2.1134	G109.871+2.114	CepA	Image	183 GHz;	7.97 (0.02)	134.0 (3.0)	109.0 (6.7)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	22 56 18.1	+62 01 46.3	109.8708	2.1134	G109.871+2.114	CepA		183 GHz;	8.37 (0.02)	131.0 (3.0)	273.0 (7.4)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	22 56 18.1	+62 01 46.3	109.8708	2.1134	G109.871+2.114	CepA		183 GHz;	10.21 (0.02)	303.4 (3.0)	358.0 (13.0)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	22 56 18.1	+62 01 46.3	109.8708	2.1134	G109.871+2.114	CepA		183 GHz;	10.77 (0.02)	214.0 (3.0)	221.0 (12.0)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	22 56 18.1	+62 01 46.3	109.8708	2.1134	G109.871+2.114	CepA		183 GHz;	11.82 (0.06)	16.4 (3.0)	9.2 (1.8)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	22 56 18.1	+62 01 46.3	109.8708	2.1134	G109.871+2.114	CepA		183 GHz;	13.05 (0.02)	72.9 (3.0)	92.2 (2.2)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	22 56 18.1	+62 01 46.3	109.8708	2.1134	G109.871+2.114	CepA		183 GHz;	24.15 (0.07)	19.8 (3.0)	18.0 (4.5)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	22 56 18.1	+62 01 46.3	109.8708	2.1134	G109.871+2.114	CepA		183 GHz;	25.96 (0.47)	9.5 (3.0)	48.4 (8.1)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	22 56 18.1	+62 01 46.3	109.8708	2.1134	G109.871+2.114	CepA		183 GHz;	26.73 (0.34)	13.8 (1.0)	189.0 (13.0)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	22 56 18.1	+62 01 46.3	109.8708	2.1134	G109.871+2.114	CepA		183 GHz;	14.22 (0.50)	5.3 (1.0)	36.6 (6.4)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
11	23 13 45.2	+61 28 9.7	111.5417	0.7768	G111.542+0.766	S158		183 GHz;	58.98 (0.52)	6.5 (1.2)	51.8 (5.2)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	23 13 45.2	+61 28 9.7	111.5417	0.7768	G111.542+0.766	S158		183 GHz;	59.30 (0.04)	14.7 (3.5)	4.4 (1.4)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
13	23 13 44	+61 26 50	111.5314	0.7571	G111.542+0.766	NGC7538S		183 GHz;	55.83 (0.59)	5.2 (1.0)	35.4 (7.5)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
14	03 25 09	+30 46 20	157.9462	-21.4539	G157.947-21.453	RNO13	Image	183 GHz;	2.48 (0.06)	15.3 (2.5)	26.8 (2.1)	IRAM	14	+H₂O -CH₃OH II +OH	SFR_MIXED		23-24 dec 1989
15	06 08 35.4	+20 39 03	189.7788	0.3448	G189.777+0.345	S252A		183 GHz;	9.64 (0.23)	9.1 (1.2)	37.2 (4.6)	IRAM	14	+H₂O -CH₃OH I +CH₃OH II +OH	SFR_MIXED		23-24 dec 1989
16	03 29 3.8	+31 16 2.6	158.3478	-20.5553	G158.347-20.556	HH7-11A	Image	183 GHz;	43.70 (0.21)	12.2 (1.3)	65.1 (7.6)	IRAM	14	+H₂O -CH₃OH I -CH₃OH II	SFR_MIXED		23-24 dec 1989
	03 29 3.8	+31 16 2.6	158.3478	-20.5553	G158.347-20.556	HH7-11A		183 GHz;	30.70 (2.04)	2.8 (1.3)	52.9 (11.6)	IRAM	14	+H₂O -CH₃OH I -CH₃OH II	SFR_MIXED		23-24 dec 1989
	03 29 3.8	+31 16 2.6	158.3478	-20.5553	G158.347-20.556	HH7-11A		183 GHz;	15.40 (0.24)	7.7 (1.3)	23.5 (4.0)	IRAM	14	+H₂O -CH₃OH I -CH₃OH II	SFR_MIXED		23-24 dec 1989
19	02 25 40	+62 05 51	133.7139	1.2146	G133.715+1.215	W3IRS5	Image	183 GHz;	13.56 (0.09)	17.5 (4.5)	12.1 (3.3)	IRAM	14	+H₂O -CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 25 40	+62 05 51	133.7139	1.2146	G133.715+1.215	W3IRS5		183 GHz;	33.95 (0.06)	18.7 (4.5)	12.9 (3.0)	IRAM	14	+H₂O -CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 25 40	+62 05 51	133.7139	1.2146	G133.715+1.215	W3IRS5		183 GHz;	37.47 (0.02)	149.0 (4.5)	279.0 (5.1)	IRAM	14	+H₂O -CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 25 40	+62 05 51	133.7139	1.2146	G133.715+1.215	W3IRS5		183 GHz;	38.42 (0.22)	26.8 (4.5)	303.0 (30.0)	IRAM	14	+H₂O -CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 25 40	+62 05 51	133.7139	1.2146	G133.715+1.215	W3IRS5		183 GHz;	39.19 (0.03)	60.6 (4.5)	39.8 (3.9)	IRAM	14	+H₂O -CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 25 40	+62 05 51	133.7139	1.2146	G133.715+1.215	W3IRS5		183 GHz;	40.44 (0.07)	22.0 (5.0)	29.1 (3.3)	IRAM	14	+H₂O -CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 25 40	+62 05 51	133.7139	1.2146	G133.715+1.215	W3IRS5		183 GHz;	41.84 (0.07)	22.3 (4.5)	22.6 (4.9)	IRAM	14	+H₂O -CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
26	02 27 4.7	+61 52 25.5	133.9489	1.0651	G133.947+1.064	W3 (H2O)	Image	183 GHz;	49.61 (0.12)	159.0 (4.0)	622.0 (27.5)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 27 4.7	+61 52 25.5	133.9489	1.0651	G133.947+1.064	W3 (H2O)		183 GHz;	48.70 (0.03)	87.8 (4.0)	124.0 (12.0)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 27 4.7	+61 52 25.5	133.9489	1.0651	G133.947+1.064	W3 (H2O)		183 GHz;	45.55 (0.42)	26.4 (4.0)	114.0 (21.0)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 27 4.7	+61 52 25.5	133.9489	1.0651	G133.947+1.064	W3 (H2O)		183 GHz;	43.17 (1.16)	13.8 (4.0)	17.0 (4.0)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 27 4.7	+61 52 25.5	133.9489	1.0651	G133.947+1.064	W3 (H2O)		183 GHz;	44.77 (0.07)	12.8 (1.5)	457.0 (2.0)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 27 4.7	+61 52 25.5	133.9489	1.0651	G133.947+1.064	W3 (H2O)		183 GHz;	30.79 (0.19)	13.5 (1.5)	51.0 (5.9)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	02 27 4.7	+61 52 25.5	133.9489	1.0651	G133.947+1.064	W3 (H2O)		183 GHz;	59.38 (0.22)	11.2 (1.5)	31.9 (5.4)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
33	19 10 13.4	+09 06 14.3	43.1668	0.0114	G43.166+0.011	W49N		183 GHz;	8.50 (0.10)	65.3 (2.2)	1107.0 (19.7)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	19 10 13.4	+09 06 14.3	43.1668	0.0114	G43.166+0.011	W49N		183 GHz;	22.40 (0.70)	9.6 (1.7)	186.0 (14.6)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	19 10 13.4	+09 06 14.3	43.1668	0.0114	G43.166+0.011	W49N		183 GHz;	28.40 (0.40)	7.8 (2.4)	102.0 (14.9)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	19 10 13.4	+09 06 14.3	43.1668	0.0114	G43.166+0.011	W49N		183 GHz;	5.70 (2.20)	8.2 (0.3)	1112.0 (21.0)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	19 10 13.4	+09 06 14.3	43.1668	0.0114	G43.166+0.011	W49N		183 GHz;	30.00 (20.0)	0.8 (0.2)	161.7 (18.0)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	19 10 13.4	+09 06 14.3	43.1668	0.0114	G43.166+0.011	W49N		183 GHz;	5.20 (0.08)	37.7 (5.3)	48.7 (3.7)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	19 10 13.4	+09 06 14.3	43.1668	0.0114	G43.166+0.011	W49N		183 GHz;	11.92 (0.16)	40.7 (6.3)	169.0 (15.7)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	19 10 13.4	+09 06 14.3	43.1668	0.0114	G43.166+0.011	W49N		183 GHz;	11.70 (0.40)	45.1 (1.2)	1295.0 (15.6)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	19 10 13.4	+09 06 14.3	43.1668	0.0114	G43.166+0.011	W49N		183 GHz;	2.35 (0.12)	8.5 (3.5)	10.1 (2.7)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	19 10 13.4	+09 06 14.3	43.1668	0.0114	G43.166+0.011	W49N		183 GHz;	8.82 (0.10)	10.3 (3.5)	13.5 (3.2)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
	19 10 13.4	+09 06 14.3	43.1668	0.0114	G43.166+0.011	W49N		183 GHz;	5.34 (0.08)	31.3 (2.1)	265.0 (5.7)	IRAM	14	+H₂O +CH₃OH I +CH₃OH II +OH	SFR		23-24 dec 1989
44	14 24 11	+25 42 13	34.2760	69.2150	G34.278+69.213	RX Boo	Image	183 GHz;	0.1	15		IRAM	14	+H₂O -CH₃OH I +OH +SiO	EVOLVED		23-24 dec 1989

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(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.line) as line,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.telescope_conf) as telescope_conf,MAX(h2o_data_all.v_step) as v_step,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.url) as url,MAX(h2o_data_all.image) as image,MAX(h2o_data_all.image2) as image2,MAX(h2o_data_all.image3) as image3,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,1 as dist_parallax,MAX(h2o_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 h2o_data_all  LEFT JOIN all_objects_withmet ON h2o_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 h2o_data_all.line=transitions."Line"  WHERE ref ilike 'CER90' 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.line,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.telescope_conf,h2o_data_all.v_step,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.url,h2o_data_all.image,h2o_data_all.image2,h2o_data_all.image3,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.dist_parallax,h2o_data_all.date_txt,line_det,type,simbad_types_cat FROM h2o_data_all   LEFT JOIN all_objects_withmet ON h2o_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 h2o_data_all.line=transitions."Line"  WHERE ref ilike 'CER90' AND detected=true AND hide=false ORDER BY detected DESC,id

Display data from paper

CER90 - Detection of 183 GHz water vapour maser emission from interstellar andcircumstellar sources.

View as list of objects

Detection table from Cernicharo et al. (1990)