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ZUC87 - H2O maser emission from stars in the IRAS point-source catalog

Short title: Zuckerman & Lo (1987)
Authors: Zuckerman, B. Lo, K. Y.
Journal: Astronomy and Astrophysics (ISSN 0004-6361), vol. 173, no. 2, Feb. 1987, p. 263-270.
Bibcode:

Non-detection table: Show non-detection table
Detection table: Show detection table (13 detection) Non-detection table: Show non-detection table (51 non-detection)
Target type: IRAS,pAGB_PN

Abstract
The authors searched for H₂O masers toward 61 red stars in the IRAS point-source catalog. Ten H₂O maser sources, roughly equally divided between pre- and post-main-sequence stars, were detected. A few may be transition objects that are evolving rapidly from red giants to planetary nebulae. One of these IRAS 1634-3814, has a very large positive radial velocity, V_LSR ≡ 140 km s^-1, although it lies in a direction where differential galactic rotation would be expected to produce negative radial velocities. The H₂O radial velocities imply large kinematic distances for some of the stars.

Abstract

The authors searched for H₂O masers toward 61 red stars in the IRAS point-source catalog. Ten H₂O maser sources, roughly equally divided between pre- and post-main-sequence stars, were detected. A few may be transition objects that are evolving rapidly from red giants to planetary nebulae. One of these IRAS 1634-3814, has a very large positive radial velocity, V_LSR ≡ 140 km s^-1, although it lies in a direction where differential galactic rotation would be expected to produce negative radial velocities. The H₂O radial velocities imply large kinematic distances for some of the stars.

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Detection table from Zuckerman & Lo (1987)

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ID	Obs. RA	Obs. Dec	l	b	Group id	Source name	Spectra	Image	Line	V_peak	F_peak	Telescope	V_step	Beam	Detection	Class	Dist. (parallax)
	(J2000)	(J2000)	(deg.)	(deg.)					H₂O	(km/s)	(Jy)		(km/s)	(arcsec)	Yes/No		(kpc)
1	02 43 28.7	+62 57 5.3	135.2780	2.7971	G135.278+2.797	IRAS 0239+6244	Spectra	Image	22 GHz;	-69.8	10.5	OVRO	2.6	107	+H₂O -CH₃OH I -CH₃OH II -OH	SFR
2	04 39 13.4	+25 53 18.2	173.8533	-13.7458	G173.853-13.744	IRAS 0436+2547	Spectra	Image	22 GHz;	11.8	9.8	OVRO	2.6	107	+H₂O	SFR_MIXED
3	05 53 44.8	+24 14 45	184.9571	-0.8520	G184.957-0.852	TAU (AFGL 5171)	Spectra	Image	22 GHz;	6.6	1	OVRO	2.6	107	+H₂O -CH₃OH II +OH	SFR
4	06 34 26.3	-05 03 37.7	215.5167	-6.0800	G215.517-6.080	AFGL 5201	Spectra	Image	22 GHz;	-59.2	2.3	OVRO	2.6	107	+H₂O +OH -SiO	EVOLVED
5	07 33 57.6	+30 30 39.9	188.7973	21.8979	G188.797+21.898	AFGL 1141	Spectra	Image	22 GHz;	-3.9	9	OVRO	2.6	107	+H₂O -CH₃OH II -OH +SiO	EVOLVED
	07 33 57.6	+30 30 39.9	188.7973	21.8979	G188.797+21.898	AFGL 1141			22 GHz;	17.1	1.1	OVRO	2.6	107	+H₂O -CH₃OH II -OH +SiO	EVOLVED
7	16 37 40.1	-38 20 17.4	344.0739	5.8462	G344.074+5.847	IRAS 1634-3814	Spectra	Image	22 GHz;	143.5	1.3	OVRO	2.6	107	+H₂O +OH -SiO	EVOLVED
	16 37 40.1	-38 20 17.4	344.0739	5.8462	G344.074+5.847	IRAS 1634-3814			22 GHz;	135.6	0.6	OVRO	2.6	107	+H₂O +OH -SiO	EVOLVED
9	19 58 31.9	+34 31 31.9	70.7757	2.6844	G70.776+2.684	IRAS 1956+3423	Spectra	Image	22 GHz;	-40.8	2.7	OVRO	2.6	107	+H₂O -CH₃OH II +OH	EVOLVED
10	20 16 21.8	+35 36 5.3	73.6522	0.1946	G73.652+0.195	IRAS 2014+3526	Spectra	Image	22 GHz;	-72.4	14	OVRO	2.6	107	+H₂O -CH₃OH I -CH₃OH II -OH	SFR
11	20 57 16.4	+02 58 46.3	51.3641	-26.1129	G51.364-26.113	U Equ	Spectra	Image	22 GHz;	-75.0	3.6	OVRO	2.6	107	+H₂O -CH₃OH II +OH -SiO	EVOLVED
12	23 17 21	+59 28 48.8	111.2355	-1.2379	G111.236-1.238	IRAS 2315+5912	Spectra	Image	22 GHz;	-51.3	12.5	OVRO	2.6	107	+H₂O +CH₃OH I -CH₃OH II -OH	SFR
	23 17 21	+59 28 48.8	111.2355	-1.2379	G111.236-1.238	IRAS 2315+5912			22 GHz;	-67.1	3	OVRO	2.6	107	+H₂O +CH₃OH I -CH₃OH II -OH	SFR

Non-detection table from Zuckerman & Lo (1987)

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ID	Obs. RA	Obs. Dec	l	b	Group id	Source name	Line	Telescope	V_step	RMS	Beam	Detection	Class
	(J2000)	(J2000)	(deg.)	(deg.)			H₂O		(km/s)	(Jy)	(arcsec)	Yes/No
1	01 17 51.6	+67 13 55.1	125.4914	4.4916	G125.491+4.491	AFGL 190	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH II -OH -SiO	SFR_MIXED
2	02 47 15.9	+60 30 44.3	136.7205	0.7792	G136.720+0.779	IRAS 0243+6018	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH II	SFR_MIXED
3	03 23 59.4	+55 10 14	143.5921	-1.4610	G143.592-1.461	IRAS 0320+5459	22 GHz;	OVRO	2.6	0.300	107	-H₂O -SiO	EVOLVED
4	03 25 8.6	+65 32 5.2	137.9704	7.2554	G137.970+7.256	AFGL 5093	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH II +OH +SiO	EVOLVED
5	04 04 18.8	-15 43 29.8	208.8487	-43.9773	G208.849-43.977	V Eri	22 GHz;	OVRO	2.6	0.300	107	-H₂O	EVOLVED
6	04 30 15.5	+35 56 57.1	164.8566	-8.5451	G164.857-8.545	IRAS 0426+3550	22 GHz;	OVRO	2.6	0.300	107	-H₂O -OH	EVOLVED
7	04 35 17.4	+62 16 23.1	145.9718	9.8959	G145.972+9.896	IRC+60144	22 GHz;	OVRO	2.6	0.300	107	-H₂O -OH	EVOLVED
8	05 00 23.9	+12 56 5.6	187.7117	-17.5741	G187.712-17.574	AFGL 5134	22 GHz;	OVRO	2.6	0.300	107	-H₂O +OH -SiO	EVOLVED
9	05 30 27.3	+25 19 56.5	181.2474	-4.7762	G181.247-4.776	IRAS 0527+2517	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH I	EVOLVED
10	05 33 44.8	+30 31 4.5	177.2893	-1.3410	G177.289-1.341	IRAS 0530+3029	22 GHz;	OVRO	2.6	0.400	107	-H₂O -CH₃OH II -OH	GALAXY
11	05 39 52.7	+46 45 46	164.1445	8.3324	G164.144+8.332	IRC+50149	22 GHz;	OVRO	2.6	0.300	107	-H₂O -OH	EVOLVED
12	05 40 27.7	-07 27 28.4	211.5808	-19.1552	G211.581-19.155	IRAS 0538-0728	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH I -CH₃OH II	SFR
13	05 59 24.9	+38 25 38.1	173.2395	7.2673	G173.239+7.267	IRC+40149	22 GHz;	OVRO	2.6	0.300	107	-H₂O +SiO	EVOLVED
14	07 16 10.3	+09 59 46.7	206.7461	9.9950	G206.746+9.995	IRAS 0713+1005	22 GHz;	OVRO	2.6	0.400	107	-H₂O -OH -SiO	EVOLVED
15	07 33 20.2	-22 10 57.7	237.3185	-1.2798	G237.319-1.280	AFGL 5235	22 GHz;	OVRO	2.6	0.200	107	-H₂O -CH₃OH II -OH	GALAXY
16	07 35 40.9	-18 48 59	234.6414	0.8339	G234.641+0.834	IRAS 0733-1842	22 GHz;	OVRO	2.6	0.400	107	-H₂O -CH₃OH II	SFR
17	07 45 15.3	-37 58 6.8	252.3943	-6.7357	G252.394-6.736	IRAS 0743-3750	22 GHz;	OVRO	2.6	0.300	107	-H₂O	EVOLVED
18	08 03 02	-36 35 50.1	253.0219	-2.9951	G253.022-2.995	AR Pup	22 GHz;	OVRO	2.6	0.700	107	-H₂O -OH	EVOLVED
19	08 22 46.3	+53 04 49.1	165.3818	34.8903	G165.382+34.890	IRAS 0818+5314	22 GHz;	OVRO	2.6	0.600	107	-H₂O	EVOLVED
20	09 00 25.4	+39 03 54.1	183.4028	41.0001	G183.403+41.000	IRAS 0857+3915	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH II	GALAXY
21	13 14 4.4	-02 48 25.1	314.1453	59.5710	G314.145+59.571	SW Vir	22 GHz;	OVRO	2.6	0.300	107	+H₂O -OH +SiO	GALAXY
22	15 15 49.1	-37 09 18.5	332.3939	17.3230	G332.394+17.323	IRAS 1512-3658	22 GHz;	OVRO	2.6	0.200	107	-H₂O	SFR
23	16 02 39.6	+47 14 22.3	74.4625	47.7846	G74.463+47.786	X Her	22 GHz;	OVRO	2.6	0.200	107	+H₂O -OH	EVOLVED
24	17 13 44.5	-37 06 6.2	349.5102	1.0566	G349.509+1.055	NGC 6302	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH II +OH	EVOLVED
25	17 18 20.1	-32 27 23.3	353.8438	2.9833	G353.844+2.984	AFGL 6815S	22 GHz;	OVRO	2.6	0.300	107	-H₂O +OH	EVOLVED
26	17 44 22.7	-31 55 39.4	357.3086	-1.3333	G357.308-1.333	AFGL 5379	22 GHz;	OVRO	2.6	0.300	107	-H₂O +OH +SiO	EVOLVED
27	17 44 54.9	+50 02 38.5	77.1325	30.8711	G77.132+30.871	AFGL 5384	22 GHz;	OVRO	2.6	0.400	107	-H₂O +OH	EVOLVED
28	17 55 53.1	-09 41 24	17.8602	7.6907	G17.860+7.691	IRAS 1753-0941	22 GHz;	OVRO	2.6	0.300	107	-H₂O +OH	EVOLVED
29	17 58 35	-17 42 30.6	11.1814	3.1584	G11.181+3.159	IRAS 1755-1742	22 GHz;	OVRO	2.6	0.300	107	-H₂O +OH +SiO	EVOLVED
30	18 11 30.6	+27 05 14	53.8348	20.1806	G53.835+20.180	IRAS 1809+2704	22 GHz;	OVRO	2.6	0.300	107	-H₂O +OH	EVOLVED
31	18 18 50	-02 45 29.4	26.7325	5.9752	G26.732+5.976	AFGL 5466	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH II +OH	EVOLVED
32	18 21 18.9	-16 22 29.2	14.9760	-0.9534	G14.976-0.953	IRAS 1818-1623	22 GHz;	OVRO	2.6	0.400	107	-H₂O -OH	EVOLVED
33	18 32 50.6	-21 09 37.3	11.9896	-5.5858	G11.989-5.585	AFGL 5501	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH II +OH	EVOLVED
34	18 34 13.5	-28 32 23.7	5.4707	-9.1599	G5.471-9.160	IRAS 1831-2834	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH II +OH	EVOLVED
35	18 35 46.9	+05 35 47.6	36.1495	6.0230	G36.149+6.026	AFGL 2199	22 GHz;	OVRO	2.6	0.200	107	-H₂O -CH₃OH II -OH	EVOLVED
36	19 00 11.2	+03 45 46	37.2774	-0.2273	G37.277-0.227	AFGL 2298	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH II	SFR_MIXED
37	19 03 6.7	-37 12 50.6	359.7668	-18.1715	G359.767-18.171	VV CrA	22 GHz;	OVRO	2.6	0.300	107	-H₂O -OH	EVOLVED
38	19 12 36	-32 50 59.5	4.7901	-18.4385	G4.789-18.438	V342 Sgr	22 GHz;	OVRO	2.6	0.300	107	-H₂O -OH +SiO	EVOLVED
39	19 13 58.7	+00 07 30.6	35.6197	-4.9562	G35.620-4.956	AFGL 2343	22 GHz;	OVRO	2.6	0.200	107	-H₂O +OH -SiO	EVOLVED
40	19 19 34	+15 16 42.3	49.6945	0.8621	G49.694+0.862	IRAS 1917+1511	22 GHz;	OVRO	2.6	0.300	107	-H₂O -OH	EVOLVED
41	19 20 35.4	+15 32 39.6	50.0449	0.7693	G50.045+0.769	IRAS 1919+1526	22 GHz;	OVRO	2.6	0.300	107	-H₂O -CH₃OH II -OH	EVOLVED
42	19 37 23.5	+20 36 54.9	56.4079	-0.3072	G56.409-0.308	IRAS 1935+2030	22 GHz;	OVRO	2.6	0.500	107	+H₂O -CH₃OH II +OH -SiO	EVOLVED
43	20 04 35	+39 18 38	75.4888	4.1758	G75.489+4.176	IRAS 2002+3910	22 GHz;	OVRO	2.6	0.300	107	+H₂O -OH	SFR_MIXED
44	20 06 22.9	+27 02 11.2	65.3171	-2.7143	G65.317-2.715	AFGL 4259	22 GHz;	OVRO	2.6	0.300	107	-H₂O +OH +SiO	EVOLVED
45	21 33 23	+56 44 34.9	98.2264	3.6934	G98.226+3.693	IRAS 2131+5631	22 GHz;	OVRO	2.6	0.200	107	-H₂O -OH -SiO	EVOLVED
46	21 56 58.3	+62 18 43.4	104.1302	5.9915	G104.130+5.991	IRAS 2155+6204	22 GHz;	OVRO	2.6	0.400	107	-H₂O -CH₃OH I -CH₃OH II +OH +SiO	EVOLVED
47	22 05 30.6	+53 21 32.7	99.6340	-1.8359	G99.634-1.836	IRAS 2203+5306	22 GHz;	OVRO	2.6	0.400	107	-H₂O -CH₃OH II +OH	EVOLVED
48	22 29 10.2	+54 51 3.7	103.3481	-2.5184	G103.348-2.518	IRAS 2227+5435	22 GHz;	OVRO	2.6	0.400	107	-H₂O -OH -SiO	EVOLVED
49	22 57 11.1	+61 56 3.4	109.9240	1.9829	G109.924+1.983	IRAS 2255+6140	22 GHz;	OVRO	2.6	0.200	107	+H₂O +CH₃OH II -OH	SFR_MIXED
50	23 28 59.1	+69 10 56.2	115.6823	7.4792	G115.682+7.479	IRAS 2326+6854	22 GHz;	OVRO	2.6	0.300	107	-H₂O -SiO	EVOLVED
51	23 34 22.6	+66 01 50.2	115.2067	4.3214	G115.207+4.321	IRAS 2332+6545	22 GHz;	OVRO	2.6	0.300	107	-H₂O +OH	EVOLVED

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 ZUC87

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