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JIA99 - SiO Masers in Stars in the Inner and Outer Galactic Disk

Interferometry data

Short title: Jiang et al. (1999)
Authors: Jiang, B. W. Deguchi, Shuji Ramesh, B.
Journal: Publications of the Astronomical Society of Japan, v.51, p.95-102.
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Detection table: Show detection table (39 detection) Non-detection table: Show non-detection table (189 non-detection)

Abstract
Observations in the J=1--0, v=1 and v=2 ^{{28}} SiO and v=0 ^{{29}} SiO maser lines were made towards 97 outer- and 19 inner-disk IRAS sources with typical IRAS colors of AGB stars. 21 new ^{{28}} SiO and 1 new ^{{29}} SiO maser sources were detected above the 5 sigma level of ~ 1 Jy with the Nobeyama 45 m telescope. Collecting all of the observational data in SiO J=1--0 maser lines taken with a 45 m telescope, a comparison is made between the outer-disk, inner-disk, and bulge samples. The samples, themselves, align a sequence of mid-infrared color, flux at 12 mu m and IRAS variability index. The detection rates are 66%, 51%, and 31%, respectively, in the bulge, inner disk, and outer disk. This fact is consistent with the tendency of increasing proportion of C-rich stars in the IRAS sample and metallicity gradient with the galactocentric distance.

Abstract

Observations in the J=1--0, v=1 and v=2 ^{{28}} SiO and v=0 ^{{29}} SiO maser lines were made towards 97 outer- and 19 inner-disk IRAS sources with typical IRAS colors of AGB stars. 21 new ^{{28}} SiO and 1 new ^{{29}} SiO maser sources were detected above the 5 sigma level of ~ 1 Jy with the Nobeyama 45 m telescope. Collecting all of the observational data in SiO J=1--0 maser lines taken with a 45 m telescope, a comparison is made between the outer-disk, inner-disk, and bulge samples. The samples, themselves, align a sequence of mid-infrared color, flux at 12 mu m and IRAS variability index. The detection rates are 66%, 51%, and 31%, respectively, in the bulge, inner disk, and outer disk. This fact is consistent with the tendency of increasing proportion of C-rich stars in the IRAS sample and metallicity gradient with the galactocentric distance.

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Detection table from Jiang et al. (1999)

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ID	Obs. RA	Obs. Dec	l	b	Source name	Line	V_peak	T_a	∫T_a dv	Date	Telescope	List	Ref.
	(J2000)	(J2000)	(deg.)	(deg.)		SiO	(km/s)	(K)	(K*km/s)
1	00 14 58	+53 14 52.2	117.419319	-9.233085	IRAS00123+5258	SiO J=1-0 v=1	-18.84	0.1	0.13	1996-05-17	NRO	NRO	JIA99
2	00 14 58	+53 14 52.2	117.419319	-9.233085	IRAS00123+5258	SiO J=1-0 v=2	-20.18	0.15	0.32	1996-05-17	NRO	NRO	JIA99
3	00 53 24.6	+65 01 48.4	123.140108	2.159163	IRAS00503+6445	SiO J=1-0 v=1	-14.55	0.7	3.95	1996-05-18	NRO	NRO	JIA99
4	00 53 24.6	+65 01 48.4	123.140108	2.159163	IRAS00503+6445	SiO J=1-0 v=2	-16.27	0.8	4.68	1996-05-18	NRO	NRO	JIA99
5	01 29 27.5	+65 11 44.4	126.908639	2.617908	IRAS01260+6456	SiO J=1-0 v=1	-124.49	0.9	1.94	1996-05-17	NRO	NRO	JIA99
6	01 29 27.5	+65 11 44.4	126.908639	2.617908	IRAS01260+6456	SiO J=1-0 v=2	-125.59	0.7	1.39	1996-05-17	NRO	NRO	JIA99
7	02 50 50.5	+52 05 5.4	140.864089	-6.580344	IRAS02473+5152	SiO J=1-0 v=1	-10.13	0.2	0.87	1996-05-16	NRO	NRO	JIA99
8	02 50 50.5	+52 05 5.4	140.864089	-6.580344	IRAS02473+5152	SiO J=1-0 v=2	-9.64	0.3	1.14	1996-05-16	NRO	NRO	JIA99
9	03 07 25.3	+50 57 46.8	143.684146	-6.346727	IRAS03038+5046	SiO J=1-0 v=1	-65.74	0.45	1.88	1996-05-12	NRO	NRO	JIA99
10	03 07 25.3	+50 57 46.8	143.684146	-6.346727	IRAS03038+5046	SiO J=1-0 v=2	-65.39	1.3	3.35	1996-05-12	NRO	NRO	JIA99
11	03 41 59.6	+55 42 15.5	145.370108	0.446957	IRAS03380+5532	SiO J=1-0 v=1	16.99	0.15	0.32	1996-05-16	NRO	NRO	JIA99
12	03 41 59.6	+55 42 15.5	145.370108	0.446957	IRAS03380+5532	SiO J=1-0 v=2	18.37	0.25	1.35	1996-05-16	NRO	NRO	JIA99
13	04 14 56.7	+48 49 16.6	153.660283	-1.521106	IRAS04112+4841	SiO J=1-0 v=1	-4.66	0.7	1.22	1996-05-18	NRO	NRO	JIA99
14	04 14 56.7	+48 49 16.6	153.660283	-1.521106	IRAS04112+4841	SiO J=1-0 v=2	-5.23	0.55	1.23	1996-05-18	NRO	NRO	JIA99
15	04 29 51.3	+38 59 33.9	162.553334	-6.531088	IRAS04264+3853	SiO J=1-0 v=1	-43.01	0.3	0.55	1996-05-13	NRO	NRO	JIA99
16	04 29 51.3	+38 59 33.9	162.553334	-6.531088	IRAS04264+3853	SiO J=1-0 v=2	-46.04	0.35	0.73	1996-05-13	NRO	NRO	JIA99
17	04 43 29.1	+34 32 18.1	167.73172	-7.460663	IRAS04402+3426	SiO J=1-0 v=1	34.74	0.15	0.44	1996-05-13	NRO	NRO	JIA99
18	04 43 29.1	+34 32 18.1	167.73172	-7.460663	IRAS04402+3426	SiO J=1-0 v=2	34.69	0.25	1.06	1996-05-13	NRO	NRO	JIA99
19	04 57 52.6	+57 30 38.2	151.519331	9.051175	IRAS04536+5726	SiO J=1-0 v=1	-37.44		9.32	1996-05-13	NRO	NRO	JIA99
20	04 57 52.6	+57 30 38.2	151.519331	9.051175	IRAS04536+5726	SiO J=1-0 v=2	-37.06		6.46	1996-05-13	NRO	NRO	JIA99
21	05 16 47.1	+45 34 3.7	162.950976	4.332296	IRAS05131+4530	SiO J=1-0 v=2	-30.47	0.85	1.44	1996-05-12	NRO	NRO	JIA99
22	20 03 8.3	+25 17 27	63.450116	-3.029871	IRAS20010+2508	SiO J=1-0 v=1	24.87	1	3.7	1996-05-17	NRO	NRO	JIA99
23	20 03 8.3	+25 17 27	63.450116	-3.029871	IRAS20010+2508	SiO J=1-0 v=2	25.39	0.5	3.12	1996-05-17	NRO	NRO	JIA99
24	20 04 21.1	+17 48 32.3	57.215606	-7.215128	IRAS20020+1739	SiO J=1-0 v=1	30.88	0.8	4.54	1996-05-18	NRO	NRO	JIA99
25	20 04 21.1	+17 48 32.3	57.215606	-7.215128	IRAS20020+1739	SiO J=1-0 v=2	32.37	0.7	2.97	1996-05-18	NRO	NRO	JIA99
26	20 04 17.3	+22 04 59.2	60.862403	-4.952261	IRAS20021+2156	SiO J=1-0 v=1	23.43	0.2	0.37	1996-05-19	NRO	NRO	JIA99
27	20 05 0.3	+28 08 0.1	66.080529	-1.869081	IRAS20029+2759	SiO J=1-0 v=1	22.47	0.5	0.7	1996-05-17	NRO	NRO	JIA99
28	20 10 33.6	+27 59 35.7	66.624624	-2.976417	IRAS20084+2750	SiO J=1-0 v=1	29.09	0.3	0.81	1996-05-17	NRO	NRO	JIA99
29	20 10 33.6	+27 59 35.7	66.624624	-2.976417	IRAS20084+2750	SiO J=1-0 v=2	29.16	0.4	1.66	1996-05-17	NRO	NRO	JIA99
30	20 16 6.2	+24 13 38.9	64.148539	-6.080833	IRAS20139+2404	SiO J=1-0 v=1	32.33	1.5	4.8	1996-05-18	NRO	NRO	JIA99
31	20 16 6.2	+24 13 38.9	64.148539	-6.080833	IRAS20139+2404	SiO J=1-0 v=2	34.03	0.7	2.7	1996-05-18	NRO	NRO	JIA99
32	20 20 12.4	+29 37 21.9	69.156475	-3.832337	IRAS20181+2927	SiO J=1-0 v=1	11.02	0.4	0.7	1996-05-17	NRO	NRO	JIA99
33	20 26 45.8	+28 23 53.2	68.965495	-5.708143	IRAS20246+2813	SiO J=1-0 v=1	18.26	0.4	2.03	1996-05-19	NRO	NRO	JIA99
34	20 26 45.8	+28 23 53.2	68.965495	-5.708143	IRAS20246+2813	SiO J=1-0 v=2	17.65	0.5	2.26	1996-05-19	NRO	NRO	JIA99
35	20 50 57.8	+42 48 4.2	83.419106	-0.888554	IRAS20491+4236	SiO J=1-0 v=1	-42.19	1.2	2.03	1996-05-19	NRO	NRO	JIA99
36	20 50 57.8	+42 48 4.2	83.419106	-0.888554	IRAS20491+4236	SiO J=1-0 v=2	-42.91	0.9	1.82	1996-05-19	NRO	NRO	JIA99
37	22 41 00	+69 46 13.9	112.034428	9.708008	IRAS22394+6930	SiO J=1-0 v=1	-42.46	0.3	1.94	1996-05-18	NRO	NRO	JIA99
38	22 41 00	+69 46 13.9	112.034428	9.708008	IRAS22394+6930	SiO J=1-0 v=2	-39.75	0.3	0.91	1996-05-18	NRO	NRO	JIA99
39	23 58 38.7	+60 53 47.9	116.554254	-1.319708	IRAS23561+6037	SiO J=1-0 v=1	-54.91	0.2	0.3	1996-05-14	NRO	NRO	JIA99

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 JIA99

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Longitude-Velocity Map is taken form Dame, Hartmann & Thaddeus (2001)

Distribution of sources from JIA99 in (l,b) histograms

Display associated data

Group name
Different Line detections
IRAS source	IRAS coordinates (RA, Dec)	IRAS source distance (arcsec)	IRAS flux density (F12,F25,F60,F100)
2MASS source	2MASS coordinates (RA, Dec)	2MASS source distance (arcsec)	2MASS magnituted (J,H,K)
GCVS source	GCVS coordinates (RA, Dec)	GCVS source distance (arcsec)	GCVS parameters
WISE source	WISE coordinates (RA, Dec)	WISE source distance (arcsec)	WISE magnitudes (w1, w2, w3, w4)
Akari IRC source	Akari IRC coordinates (RA, Dec)	Akari IRC source distance (arcsec)	Akari IRC fluxes (S09, S18)
Akari FIS source	Akari FIS coordinates (RA, Dec)	Akari FIS source distance (arcsec)	Akari FIS fluxes (S65, S90, S140, S160)
Continuum source	Continuum coordinates (RA, Dec)	Continuum source distance (arcsec)	Continuum parameters
Bolocam GPS	BGPS coordinates (RA, Dec)	BGPS source distance (arcsec)	BGPS parameters
EGO source	EGO coordinates (RA, Dec)	EGO source distance (arcsec)	EGO parameters
Select all	Select all	Select all	Select all

View images

DSS (optical)	2MASS (JHK)	WISE (4-22 um)	IRAC (3-8 um)	GLIMPSE 360 (3.6-4.5 um)	PACS color (70-160 um)	SPIRE color (250-500 um)
AKARI color (60-160 um)	NVSS (1.4 GHz)	SDSS (optical+NIR)	Image size: arcsec (default is 120 arcsec)
			Image size: arcsec (default is 120 arcsec)

Position of H₂O maser detection

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(sio_data.ra_hms) as ra_hms,MAX(sio_data.dec_dms) as dec_dms,MAX(sio_data.source_name) as source_name,MAX(sio_data.ra) as ra,MAX(sio_data.dec) as dec,MAX(sio_data.l) as l,MAX(sio_data.b) as b,MAX(sio_data.vlow) as vlow,MAX(sio_data.vup) as vup,MAX(sio_data.vpeak) as vpeak,MAX(sio_data.vpeak_e) as vpeak_e,MAX(sio_data.vpeak2) as vpeak2,MAX(sio_data.vpeak2_e) as vpeak2_e,MAX(sio_data.dv) as dv,MAX(sio_data.other_name) as other_name,MAX(sio_data.peak) as peak,MAX(sio_data.peak_e) as peak_e,MAX(sio_data.peak2) as peak2,MAX(sio_data.peak2_e) as peak2_e,MAX(sio_data.int) as int,MAX(sio_data.int_e) as int_e,MAX(sio_data.rms) as rms,MAX(sio_data.date) as date,MAX(sio_data.date2) as date2,MAX(sio_data.telescope_ref) as telescope_ref,MAX(sio_data.units) as units,MAX(sio_data.beam) as beam,MAX(sio_data.ref) as ref,MAX(sio_data.list_ref) as list_ref,MAX(sio_data.ascii) as ascii,MAX(sio_data.image) as image,MAX(sio_data.id) as id,MAX(sio_data.date_txt) as date_txt,MAX(sio_data.line) as line FROM sio_data  WHERE ref ilike 'JIA99' AND detected=true AND hide=false GROUP BY ref

select sio_data.ra_hms,sio_data.dec_dms,sio_data.source_name,sio_data.ra,sio_data.dec,sio_data.l,sio_data.b,sio_data.vlow,sio_data.vup,sio_data.vpeak,sio_data.vpeak_e,sio_data.vpeak2,sio_data.vpeak2_e,sio_data.dv,sio_data.other_name,sio_data.peak,sio_data.peak_e,sio_data.peak2,sio_data.peak2_e,sio_data.int,sio_data.int_e,sio_data.rms,sio_data.date,sio_data.date2,sio_data.telescope_ref,sio_data.units,sio_data.beam,sio_data.ref,sio_data.list_ref,sio_data.ascii,sio_data.image,sio_data.id,sio_data.date_txt,sio_data.line FROM sio_data   WHERE ref ilike 'JIA99' AND detected=true AND hide=false ORDER BY detected DESC,id