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SIV90 - An OH survey of Mira-like objects from the IRAS point source catalog

Short title: Sivagnanam et al. (1990)
Authors: Sivagnanam, P. Le Squeren, A. M. Minh, F. Tran Braz, M. A.
Journal: Astronomy and Astrophysics (ISSN 0004-6361), vol. 233, no. 1, July 1990, p. 112-120.
Bibcode:

Abstract
An OH survey was performed of IRAS sources that present IR colors similar to Mira stars and for which an LRS observation was available. A total of 143 objects were observed in the 1612 and 1667 MHz lines: OH masers were found in 36 objects. The aim of this work is to characterize a large number of evolved circumstellar envelopes from microwave spectra, and to explore the evolution of Asymptotic Giant Branch objects. Special attention is given to the comparison of the objects found in the present study with the known Miras. The kinematics of the envelopes that show peculiar OH spectra is discussed.	Target sources: IRAS Comments: Velocity resolution: 0.60 km/s Upper limit for non-detections: 0.13 Jy (3σ)

Abstract

An OH survey was performed of IRAS sources that present IR colors similar to Mira stars and for which an LRS observation was available. A total of 143 objects were observed in the 1612 and 1667 MHz lines: OH masers were found in 36 objects. The aim of this work is to characterize a large number of evolved circumstellar envelopes from microwave spectra, and to explore the evolution of Asymptotic Giant Branch objects. Special attention is given to the comparison of the objects found in the present study with the known Miras. The kinematics of the envelopes that show peculiar OH spectra is discussed.

Target sources:
IRAS

Comments:
Velocity resolution: 0.60 km/s
Upper limit for non-detections: 0.13 Jy (3σ)

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Detection table from Sivagnanam et al. (1990)

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ID	Obs. RA	Obs. Dec	l	b	Group id	Source name	Frequency	V_range	V_peak	F_peak	List	Detection	Class	Dist. (parallax)	Ref.
	(J2000)	(J2000)	(deg.)	(deg.)			(MHz)	(km/s)	(km/s)	(Jy)		Yes/No		(kpc)
1	02 00 44.1	+58 59 03	131.7680	-2.6936	G131.768-2.694	IRAS 01572+5844	1612	16.9	-19.8	0.174	ENG15	-H₂O +OH	EVOLVED		SIV90
2	04 24 40.2	+48 07 24	155.2981	-0.8858	G155.298-0.886	IRAS 04209+4800	1612	26.4	-26.4	0.076	ENG15	+H₂O +OH +SiO	EVOLVED		SIV90
3	07 21 23.4	-28 31 58	241.6538	-6.6561	G241.654-6.656	IRAS 07193-2826	1612	8.7	8.7	0.179	ENG15	+OH	EVOLVED		SIV90
4	13 27 17.3	-25 02 14	313.1286	37.1237	G313.129+37.124	IRAS 13245-2446	1612	8.1	18.3	0.176	ENG15	+OH -SiO	EVOLVED		SIV90
5	14 28 8.8	-33 00 02	325.3259	25.6314	G325.327+25.631	IRAS 14251-3246	1612	17.4	-30.8	0.309	ENG15	-H₂O +OH +SiO	EVOLVED		SIV90
6	15 00 1.8	-21 47 03	338.5862	32.0393	G338.586+32.039	IRAS 14571-2135	1612	7.6	30.8	0.207	ENG15	+OH +SiO	EVOLVED		SIV90
7	15 28 43.7	+03 49 43	8.1035	45.8400	G8.104+45.840	IRAS 15262+0400	1612	12.4	38.0	0.135	ENG15	+H₂O +OH +SiO	EVOLVED		SIV90
8	16 05 28.3	+42 10 31	66.8770	47.9976	G66.877+47.998	IRAS 16037+4218	1612	6.4	-2.8	0.273	ENG15	+OH +SiO	EVOLVED		SIV90
9	16 12 00	-17 03 14	356.5649	24.3049	G356.565+24.305	IRAS 16091-1655	1612	14.0	41.8	1.260	ENG15	+OH +SiO	EVOLVED		SIV90
10	16 20 35.2	-32 09 36	346.2648	12.6012	G346.265+12.601	IRAS 16173-3202	1612	18.0	-70.9	0.859	ENG15	+OH +SiO	EVOLVED		SIV90
11	16 50 10.7	-32 16 58	350.3823	7.8305	G350.382+7.831	IRAS 16469-3211	1612	11.6	34.9	0.428	ENG15	+OH	EVOLVED		SIV90
12	16 51 49.3	-30 19 50	352.1403	8.7837	G352.140+8.784	IRAS 16486-3014	1612	20.0	40.0	1.013	ENG15	+OH	EVOLVED		SIV90
13	16 59 26.9	-35 04 27	349.3964	4.5826	G349.396+4.583	IRAS 16561-3459	1612	15.1	15.1	0.243	ENG15	+OH	EVOLVED		SIV90
14	17 03 6.5	-20 33 24	1.6314	12.6664	G1.632+12.665	IRAS 17001-2029	1612	79.6	79.6	0.428	ENG15	+OH +SiO	EVOLVED		SIV90
15	17 13 41.5	-28 07 50	356.8088	6.2978	G356.809+6.298	IRAS 17105-2804	1612	14.5	49.4	0.516	ENG15	+OH	EVOLVED		SIV90
16	17 27 5.4	-28 15 30	358.3830	3.7934	G358.383+3.793	IRAS 17239-2812	1612	41.3	-47.6	1.476	ENG15	+OH +SiO	SFR_MIXED		SIV90
17	17 34 49.7	-34 16 36	354.2552	-0.8897	G354.255-0.890	IRAS 17315-3414	1612	29.6	-5.8	1.698	ENG15	+OH	EVOLVED		SIV90
18	17 48 23.3	-16 01 59	11.4049	6.1090	G11.405+6.109	IRAS 17455-1601	1612	24.5	6.9	0.146	ENG15	+OH	EVOLVED		SIV90
19	17 52 51.4	-31 08 09	358.9185	-2.4743	G358.919-2.474	IRAS 17496-3107	1612	31.4	9.3	0.344	ENG15	+OH	EVOLVED		SIV90
20	17 58 34.3	-35 54 50	355.3645	-5.8928	G355.364-5.893	IRAS 17552-3554	1612	43.5	43.5	0.219	ENG15	+OH	EVOLVED		SIV90
21	18 09 24.2	-31 39 28	0.2028	-5.8057	G0.203-5.806	IRAS 18061-3140	1612	72.1	-72.1	0.632	ENG15	+OH	EVOLVED		SIV90
22	18 57 20.8	+09 09 40	41.7613	2.8630	G41.761+2.863	IRAS 18549+0905	1612	22.6	8.1	1.276	ENG15	+H₂O +OH +SiO	EVOLVED		SIV90
23	19 22 16.3	+05 06 58	41.0211	-4.4873	G41.021-4.486	IRAS 19198+0501	1612	12.8	-43.0	0.555	ENG15	+OH +SiO	EVOLVED		SIV90
24	19 33 34.4	+11 37 02	48.0892	-3.8732	G48.089-3.873	IRAS 19312+1130	1612	25.5	53.5	0.102	ENG15	-H₂O +OH +SiO	EVOLVED		SIV90
25	20 42 18.7	-08 15 32	38.2823	-28.3701	G38.283-28.370	IRAS 20396-0826	1612	6.4	-53.5	1.418	ENG15	+OH +SiO	EVOLVED		SIV90
26	20 57 16.3	+02 58 46	51.3639	-26.1127	G51.364-26.113	IRAS 20547+0247	1612	4.7	-80.4	0.438	ENG15	+H₂O -CH₃OH II +OH -SiO	EVOLVED		SIV90
27	21 08 47.4	+01 10 13	51.3761	-29.5117	G51.377-29.512	IRAS 21062+0058	1612	9.8	15.1	0.328	ENG15	+H₂O +OH +SiO	EVOLVED		SIV90
28	22 07 20	+40 48 42	92.3910	-12.1311	G92.391-12.131	IRAS 22052+4034	1612	18.0	-34.9	0.334	ENG15	+H₂O +OH	EVOLVED		SIV90
29	22 12 15.4	+51 35 03	99.4403	-3.8774	G99.440-3.877	IRAS 22103+5120	1612	57.7	-57.7	0.139	ENG15	-H₂O +OH +SiO	EVOLVED		SIV90
30	22 48 14.1	+69 58 29	112.6884	9.5924	G112.688+9.592	IRAS 22466+6942	1612	10.4	-51.1	0.686	ENG15	+H₂O +OH +SiO	EVOLVED		SIV90
31	22 54 31.9	+60 49 38	109.1606	1.1203	G109.160+1.121	IRAS 22525+6033	1612	8.7	-65.1	0.111	ENG15	+H₂O +OH +SiO	EVOLVED		SIV90
32	23 37 40	+58 50 47	113.5020	-2.6681	G113.502-2.668	IRAS 23352+5834	1612	8.1	-94.1	0.677	ENG15	-H₂O +OH +SiO	EVOLVED		SIV90
33	03 52 55.1	-09 10 09	198.9889	-43.6230	G198.989-43.623	IRAS 03505-0919	1667	20.8	-20.8	0.161	ENG15	+OH	EVOLVED		SIV90
34	04 24 40.2	+48 07 24	155.2981	-0.8858	G155.298-0.886	IRAS 04209+4800	1667	26.4	-26.4	0.557	ENG15	+H₂O +OH +SiO	EVOLVED		SIV90
35	13 27 17.3	-25 02 14	313.1286	37.1237	G313.129+37.124	IRAS 13245-2446	1667	8.1	18.3	0.149	ENG15	+OH -SiO	EVOLVED		SIV90
36	15 00 1.8	-21 47 03	338.5862	32.0393	G338.586+32.039	IRAS 14571-2135	1667	7.6	30.8	0.086	ENG15	+OH +SiO	EVOLVED		SIV90
37	15 25 47.7	-36 13 56	334.6663	16.9547	G334.666+16.955	IRAS 15226-3603	1667	16.3	-65.7	0.457	ENG15	+OH +SiO	EVOLVED		SIV90
38	15 28 43.7	+03 49 43	8.1035	45.8400	G8.104+45.840	IRAS 15262+0400	1667	12.4	38.0	0.121	ENG15	+H₂O +OH +SiO	EVOLVED		SIV90
39	16 12 00	-17 03 14	356.5649	24.3049	G356.565+24.305	IRAS 16091-1655	1667	41.8	41.8	0.097	ENG15	+OH +SiO	EVOLVED		SIV90
40	16 50 10.7	-32 16 58	350.3823	7.8305	G350.382+7.831	IRAS 16469-3211	1667	11.6	34.9	0.194	ENG15	+OH	EVOLVED		SIV90
41	17 03 6.5	-20 33 24	1.6314	12.6664	G1.632+12.665	IRAS 17001-2029	1667	79.6	79.6	0.224	ENG15	+OH +SiO	EVOLVED		SIV90
42	18 18 49.9	-02 45 29	26.7324	5.9757	G26.732+5.976	IRAS 18162-0246	1667	6.8	6.8	0.177	ENG15	-H₂O -CH₃OH II +OH	EVOLVED		SIV90
43	18 57 20.8	+09 09 40	41.7613	2.8630	G41.761+2.863	IRAS 18549+0905	1667	22.6	8.1	0.113	ENG15	+H₂O +OH +SiO	EVOLVED		SIV90
44	20 42 18.7	-08 15 32	38.2823	-28.3701	G38.283-28.370	IRAS 20396-0826	1667	53.5	-53.5	0.219	ENG15	+OH +SiO	EVOLVED		SIV90
45	20 57 16.3	+02 58 46	51.3639	-26.1127	G51.364-26.113	IRAS 20547+0247	1667	4.7	-80.4	0.122	ENG15	+H₂O -CH₃OH II +OH -SiO	EVOLVED		SIV90
46	20 56 24.5	+52 56 59	91.7977	4.9221	G91.798+4.922	IRAS 20549+5245	1667	4.8	-4.8	0.197	ENG15	-H₂O -CH₃OH II +OH +SiO	EVOLVED		SIV90
47	22 07 20	+40 48 42	92.3910	-12.1311	G92.391-12.131	IRAS 22052+4034	1667	18.0	-34.9	0.185	ENG15	+H₂O +OH	EVOLVED		SIV90
48	22 54 31.9	+60 49 38	109.1606	1.1203	G109.160+1.121	IRAS 22525+6033	1667	8.7	-65.1	0.256	ENG15	+H₂O +OH +SiO	EVOLVED		SIV90
49	23 37 40	+58 50 47	113.5020	-2.6681	G113.502-2.668	IRAS 23352+5834	1667	94.1	-94.1	0.109	ENG15	-H₂O +OH +SiO	EVOLVED		SIV90

Non-detection table from Sivagnanam et al. (1990)