2007AJ....133..496C

Query : 2007AJ....133..496C

2007AJ....133..496C - Astron. J., 133, 496-503 (2007/February-0)

Photometric study of galaxies with OH megamasers in the infrared.

CHEN P.S., SHAN H.G. and GAO Y.F.

Abstract (from CDS):

OH megamasers are the most luminous masers in the universe. The total of 109 OH megamaser (OHM) galaxies known so far have been collected, and cross-identifications of those OHM galaxies with Two Micron All Sky Survey (2MASS) sources are made in this paper. Using 2MASS and IRAS data, the infrared properties of OHM-detected and nondetected sources are compared. It is shown that the main difference between those two kinds of sources is the infrared color from 25 to 60 µm. Statistically, the OHM-detected sources have redder colors and steeper spectral indices in the 25-60 µm region than the nondetected sources. In addition, considering the spectral types, the properties of the OHM galaxies in the near-infrared and far-infrared are discussed. It is found that Seyfert 1 and Seyfert 2 sources with hidden broad-line regions (BLRs) have redder colors and steeper spectral indices than other sources, including LINER, composite spectrum nucleus, and H II sources in the near-infrared region, whereas the latter have redder colors and steeper spectral indices than the Seyfert 1 and Seyfert 2 sources with hidden BLRs in the far-infrared. It is also found that almost all sources either with or without an identified spectral type show a starburst-dominated feature in the far-infrared, while a considerable number of sources, in particular Seyfert 1 and Seyfert 2 sources with hidden BLRs, show an active galactic nucleus-dominated feature in the near-infrared. Furthermore, as far-infrared radiation at 35 and 53 µm is likely responsible for the OH maser pumping in OHM galaxies, the pumping efficiencies in the infrared are also analyzed in this paper. It is found that, statistically, the pumping efficiencies increase with far-infrared color. It is also found that, statistically, the OH peak fluxes are not proportional to the related infrared fluxes at either 35 or 53 µm. This result implies that the pump lines are optically thin and the pump sources are unsaturated.

Abstract Copyright: ∼

Journal keyword(s): Galaxies: Nuclei - Galaxies: Starburst - Infrared: Galaxies - ISM: Masers - Radio Lines: Galaxies

VizieR on-line data: <Available at CDS (J/AJ/133/496): table1.dat table2.dat>

Simbad objects: 152

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Number of rows : 152
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 NPM1G +40.0002 Sy2 00 08 20.3675391072 +40 37 55.922085984     16.8     ~ 47 0
2 NVSS J003600-271535 rG 00 36 00.3760623744 -27 15 33.890537268   17.18       ~ 42 0
3 NGC 253 SyG 00 47 33.134 -25 17 19.68   8.03   6.94 8.1 ~ 3588 2
4 Mrk 1502 Sy1 00 53 34.9331107632 +12 41 35.929269132   14.41 14.03     ~ 1242 1
5 LAMOST J012343.44+354055.1 G 01 23 43.4455106184 +35 40 55.029467568           ~ 11 0
6 IRAS 01364-1042 LIN 01 38 52.86288 -10 27 11.5848   16.77   15.74   ~ 132 0
7 ZW III 35 Sy2 01 44 30.516 +17 06 09.18   15.24 14.81     ~ 261 1
8 IRAS 01562+2527 rG 01 59 02.62587 +25 42 36.7670           ~ 21 0
9 Mrk 1014 Sy1 01 59 50.2534701768 +00 23 40.864244784   16.08 15.87     ~ 606 0
10 IRAS 02183+2254 FIR 02 21 10.0 +23 08 26           ~ 5 0
11 2MASX J02320486+3152448 G 02 32 04.8386573592 +31 52 45.207353100           ~ 9 0
12 M 77 Sy2 02 42 40.7091669408 -00 00 47.859690204 9.70 9.61 8.87 10.1 9.9 ~ 4897 2
13 NVSS J024346+040636 rG 02 43 46.05240 +04 06 38.1960           ~ 44 1
14 2MASX J02513583+4315117 LIN 02 51 35.8187772168 +43 15 11.772126504   18.09 17.36     ~ 60 0
15 IRAS 02524+2046 AGN 02 55 17.12208 +20 58 57.6588           ~ 23 0
16 Z 463-51 G 03 08 30.7190875152 +20 46 20.121735648   15.1       ~ 50 0
17 NVSS J032824-141207 rG 03 28 24.3444674448 -14 12 07.277097384   16.68   15.55   ~ 20 0
18 NGC 1365 Sy1 03 33 36.458 -36 08 26.37 10.48 10.08 9.63 8.79 9.7 ~ 1987 2
19 IRAS 03521+0028 AGN 03 54 42.14640 +00 37 03.3280           ~ 104 0
20 IRAS 03566+1647 Sy2 03 59 28.4928678264 +16 56 24.662593284           ~ 15 0
21 IRAS 04121+0223 AGN 04 14 47.47002720 +02 30 41.3147520           ~ 25 0
22 Z 393-40 AG? 04 35 48.4302410280 +02 15 29.990712312   15.6       ~ 49 0
23 ESO 203-1 AGN 04 46 49.4729569488 -48 33 30.480074640   16.40   15.51   ~ 73 0
24 IRAS 05100-2425 rG 05 12 09.179 -24 21 56.47   16.46 15.0 15.28   ~ 35 1
25 IRAS 05189-2524 Sy2 05 21 01.3994605776 -25 21 45.321827832   15.47 14.75     ~ 545 0
26 MCG+10-09-002 Sy2 05 45 47.836 +58 42 03.83   16.0       ~ 110 2
27 NVSS J062222-364743 rG 06 22 22.602 -36 47 44.67   17.77   16.69   ~ 18 1
28 IRAS 06487+2208 rG 06 51 45.73536 +22 04 27.3180           ~ 36 0
29 IRAS 07163+0817 AGN 07 19 05.48483760 +08 12 06.4583640           ~ 18 0
30 IRAS 07572+0533 LIN 07 59 59.7425607048 +05 24 51.495550020           ~ 23 0
31 NVSS J080947+050108 rG 08 09 47.236 +05 01 09.36           ~ 28 0
32 IRAS 08201+2801 LIN 08 23 12.6165437400 +27 51 39.639008772           ~ 63 0
33 IRAS 08232+0058 G 08 25 47.5569760141 +00 49 03.896022264           ~ 5 0
34 IRAS 08279+0956 rG 08 30 39.31656 +09 46 36.9336           ~ 19 0
35 IRAS 08449+2332 PaG 08 47 50.18547 +23 21 09.7780           ~ 30 0
36 IRAS 08474+1813 Sy2 08 50 18.34248 +18 02 01.2408   19.99 19.03     ~ 41 0
37 IRAS 08559+1053 Sy2 08 58 41.7769654542 +10 41 21.877217105           ~ 60 0
38 IRAS 09039+0503 LIN 09 06 34.0537343016 +04 51 27.447987744           ~ 86 0
39 Z 289-11 Sy2 09 35 51.6045544584 +61 21 11.589382368   15.20 15.50     ~ 617 2
40 2MASS J09554997+1416067 Sy2 09 55 49.98722 +14 16 06.9015           ~ 20 1
41 IRAS 09531+1430 MIR 09 55 50.26251 +14 16 07.8989           ~ 22 0
42 IRAS 09539+0857 Sy2 09 56 34.33800 +08 43 06.2472       20.90   ~ 63 0
43 IC 2545 Sy1 10 06 04.581 -33 53 05.55   15.27 14.27 14.25   ~ 117 0
44 IRAS 10036+2740 rG 10 06 26.31960 +27 25 46.4840           ~ 44 1
45 NVSS J102000+081335 rG 10 20 00.1849825704 +08 13 33.648546108   17.5       ~ 167 1
46 IRAS 10339+1548 Sy2 10 36 37.9423862832 +15 32 41.961280452           ~ 32 0
47 IRAS 10378+1109 Sy1 10 40 29.1640944744 +10 53 18.202070076   17.79 17.18     ~ 115 1
48 LEDA 32516 LIN 10 51 03.67 -15 03 19.8           ~ 47 0
49 APG 148 IG 11 03 53.89153 +40 50 59.8850   14.29       ~ 190 1
50 IRAS 11029+3130 LIN 11 05 37.53576 +31 14 32.1432           ~ 54 0
51 IRAS 11069+2711 rG 11 09 37.43149 +26 55 15.6924           ~ 35 0
52 IRAS 11180+1623 LIN 11 20 41.77536 +16 06 56.5668           ~ 42 0
53 NGC 3690 IG 11 28 31.0 +58 33 41   13.19 12.86     ~ 1015 4
54 NGC 3690B GiP 11 28 31.02 +58 33 40.7   11.8       ~ 635 4
55 NGC 3690NE AGN 11 28 33.07 +58 33 54.2   11.8       ~ 635 4
56 MCG-06-26-013 EmG 11 53 11.722 -39 07 48.72   13.30   11.86   ~ 203 1
57 IRAS 11524+1058 LIN 11 55 05.13672 +10 41 22.8012           ~ 26 0
58 IRAS 12005+0009 Sy1 12 03 04.4290327200 -00 07 27.444831888   18.70 18.09     ~ 31 0
59 IRAS 12018+1941 Sy2 12 04 24.5432777064 +19 25 09.773024772           ~ 89 0
60 IRAS 12032+1707 LIN 12 05 47.7089284392 +16 51 08.355094704   18.758   17.327   ~ 68 0
61 IRAS 12112+0305 PaG 12 13 45.98880 +02 48 39.9600           ~ 373 0
62 [CGM90] IRAS 12112+0305 NE rG 12 13 46.10735 +02 48 41.4959           ~ 369 0
63 IRAS 12162+1047 G 12 18 47.7615387978 +10 31 14.133681912           ~ 16 0
64 NGC 4355 Sy2 12 26 54.6206739120 -00 52 39.421212996   14.21 13.37     ~ 527 2
65 IRAS 12514+1027 Sy2 12 54 00.8097492312 +10 11 12.237857124   19.03 18.27     ~ 57 0
66 Z 294-4 Sy1 12 56 14.2341182928 +56 52 25.238373852   14.68 13.84     ~ 2096 3
67 IRAS 12548+2403 rG 12 57 20.05007 +23 47 46.0720           ~ 15 0
68 NGC 5010 GiG 13 12 26.331 -15 47 52.64   14.3       ~ 85 0
69 IC 860 LIN 13 15 03.51 +24 37 07.8   14.8       ~ 236 0
70 IRAS 13218+0552 Sy2 13 24 19.8862877976 +05 37 04.693531332   19.31 18.73 17.41   ~ 130 0
71 NAME Centaurus A BLL 13 25 27.61521044 -43 01 08.8050291   8.18 6.84 6.66   ~ 4774 3
72 NVSS J132732+473906 rG 13 27 32.6689899240 +47 39 03.503011572           ~ 28 0
73 Z 271-60 Sy2 13 44 42.1883001099 +55 53 13.596220922   15.68 14.91     ~ 958 3
74 LEDA 1681523 G 13 46 39.265 +23 06 18.15           ~ 21 0
75 PKS 1345+12 Sy2 13 47 33.36161873 +12 17 24.2398927   19.28 18.44 15.718   ~ 652 2
76 IRAS 13539+2920 rG 13 56 10.01233 +29 05 35.5160   17.23       ~ 70 0
77 SDSS J135646.10+102609.0 Sy2 13 56 46.106 +10 26 09.09   18.90 18.11     ~ 95 0
78 IRAS 14043+0624 Sy1 14 06 49.8223642584 +06 10 36.069658464           ~ 19 0
79 IRAS 14059+2000 rG 14 08 18.72720 +19 46 22.7280           ~ 28 0
80 IRAS 14060+2919 rG 14 08 19.0356546744 +29 04 47.143121916           ~ 68 0
81 IRAS 14070+0525 Sy2 14 09 31.26096 +05 11 31.3548     17.00     ~ 78 0
82 LEDA 84144 Sy1 14 22 30.3441895296 +29 52 24.178323540   17.62 17.12     ~ 37 1
83 IRAS 14202+2615 rG 14 22 31.3873621186 +26 02 05.256515503           ~ 53 0
84 NVSS J142503+272908 rG 14 25 03.871 +27 29 10.84           ~ 10 0
85 IRAS 14312+2825 Sy2 14 33 27.5181065472 +28 11 59.739397224   18.19 17.52     ~ 23 0
86 NVSS J144244+262134 rG 14 42 44.8293689256 +26 21 30.319683768   17.94       ~ 23 0
87 IRAS F14406+2216 G 14 42 50.7 +22 03 56           ~ 4 0
88 2MASX J14481604+1733055 LIN 14 48 16.048 +17 33 05.93           ~ 22 0
89 IRAS 14488+3520 Sy1 14 50 54.1660789584 +35 08 37.872832056   17.79 17.21     ~ 24 0
90 IRAS 14553+1245 rG 14 57 42.5066364960 +12 33 21.139165044           ~ 22 0
91 NVSS J145936+324459 rG 14 59 36.548 +32 44 59.23   17.36       ~ 25 0
92 IRAS 14586+1431 rG 15 01 02.22230 +14 20 02.9900           ~ 14 0
93 IRAS 15001+1433 Sy2 15 02 31.9755844913 +14 21 34.926031528   20.69 20.13     ~ 68 0
94 IRAS 15069+1808 Sy1 15 09 13.7937691872 +17 57 09.962110728   17.37 17.06     ~ 45 0
95 NGC 5861 Sy2 15 09 16.09127 -11 19 17.9800   13.34 12.62 11.03 11.5 ~ 186 0
96 Z 49-57 rG 15 13 13.1083645335 +07 13 32.099256087   15.5       ~ 252 1
97 NVSS J151758+273614 rG 15 17 58.517 +27 36 15.90           ~ 10 0
98 NAME CG 1517+39 rG 15 19 47.088 +39 45 36.65   16.75 16.12     ~ 40 1
99 IRAS 15206+3631 Sy1 15 22 34.8562443384 +36 20 58.716100932           ~ 14 0
100 IRAS 15206+3342 Sy2 15 22 38.104 +33 31 35.90           ~ 111 0
101 IRAS 15225+2350 rG 15 24 43.8702463632 +23 40 10.269173100           ~ 55 0
102 IRAS F15224+1033 rG 15 24 51.1870425888 +10 22 48.774218952           ~ 19 0
103 2MASX J15254953+0522483 LIN 15 25 49.5464595360 +05 22 48.616189824           ~ 32 0
104 2MASX J15265942+3558372 LIN 15 26 59.44451 +35 58 37.0521   15.61       ~ 295 1
105 2MASX J15272771-0955416 LIN 15 27 27.7454360616 -09 55 42.079346796   16.38 15.5 14.91   ~ 30 0
106 IC 1127 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 3090 4
107 IRAS 15587+1609 PaG 16 01 02.79385 +16 01 03.5838           ~ 18 0
108 IRAS 16075+2838 Sy2 16 09 33.4089 +28 30 58.367   18.30 17.63     ~ 25 0
109 IRAS 16100+2528 G 16 12 05.4137851199 +25 20 23.575637364           ~ 18 0
110 Z 223-53 GiC 16 16 11.221 +42 23 59.33   15.2       ~ 23 0
111 IRAS 16142+0321 FIR 16 16 43.3 +03 14 23           ~ 4 0
112 LEDA 2817004 Sy2 16 18 09.4114 +01 39 20.951           ~ 44 1
113 PN A66 39 PN 16 27 33.7199223168 +27 54 33.471380376   15.27 15.60     DAO.70 132 0
114 LEDA 84754 G 16 30 29.2417625064 +28 10 51.732283980           ~ 11 0
115 IRAS 16300+1558 Sy2 16 32 21.41352 +15 51 45.8280   18.72 18.06     ~ 64 0
116 LEDA 58817 Sy1 16 42 40.1747908920 -09 43 18.848119476   16.77       ~ 106 1
117 SDSS J164914.09+342513.1 G 16 49 14.09177 +34 25 13.1998           ~ 55 0
118 IRAS 16474+3430 PaG 16 49 14.20173 +34 25 09.6170           ~ 61 0
119 IRAS F16544+3212 G 16 56 24.4 +32 07 57           ~ 5 0
120 IRAS 17160+2006 G 17 18 16.2402564088 +20 02 55.690425635           ~ 13 0
121 LEDA 60189 LIN 17 23 21.96264 -00 17 00.8088   15.1       ~ 454 0
122 Z 171-22 G 17 54 29.392 +32 53 14.22   14.3       ~ 60 1
123 IRAS 17540+2935 AGN 17 55 56.1570262128 +29 35 26.156800140           ~ 21 0
124 2MASX J18061302+2141351 G 18 06 13.0144703040 +21 41 35.318972040           ~ 7 0
125 NVSS J181700+155449 rG 18 17 00.2654063344 +15 54 49.488072626           ~ 12 1
126 IRAS 18368+3549 Sy2 18 38 35.40744 +35 52 19.9884           ~ 40 0
127 2MASS J18575262-3714402 Y*? 18 57 52.63 -37 14 40.1           ~ 18 0
128 IRAS 18588+3517 AGN 19 00 41.16624 +35 21 26.3052           ~ 29 0
129 [VV2000] J201329.8-414735 QSO 20 13 29.55552 -41 47 35.0592   17.0       ~ 141 2
130 IRAS 20248+1734 G 20 27 08.0944591889 +17 44 22.223367555           ~ 16 0
131 IRAS 20286+1846 LIN 20 30 54.48096 +18 56 37.5648           ~ 23 0
132 IRAS 20450+2140 G 20 47 14.34813 +21 51 12.6290           ~ 16 0
133 Z 448-16 G 20 51 25.9006902384 +18 58 04.274181552   14.8       ~ 36 0
134 Z 448-20 G 20 57 23.62800 +17 07 44.5980   15.2       ~ 190 0
135 IRAS 21077+3358 AGN 21 09 50.66808 +34 10 34.1184           ~ 23 0
136 IRAS 21272+2514 Sy2 21 29 29.40072 +25 27 54.4140           ~ 35 0
137 Z 530-8 GiG 22 04 36.218 +42 19 37.50   15.7       ~ 55 1
138 IRAS 22055+3024 LIN 22 07 49.6887589920 +30 39 39.880479456           ~ 27 0
139 NVSS J221134-181704 rG 22 11 33.80928 -18 17 06.4608   18.38       ~ 39 0
140 IRAS 22116+0437 rG 22 14 10.4475776352 +04 52 26.379186636           ~ 24 0
141 NAME South America rG 22 51 49.27872 -17 52 24.0600   16.97       ~ 348 3
142 IRAS F23019+3405 Sy2 23 04 21.2033243553 +34 21 47.482753704           ~ 20 0
143 IRAS F23028+0725 rG 23 05 19.8956999688 +07 41 43.187890740           ~ 16 0
144 NVSS J230735+041559 rG 23 07 35.801 +04 16 02.01           ~ 18 0
145 IRAS 23129+2548 LIN 23 15 21.39960 +26 04 32.2536           ~ 54 0
146 IC 5298 Sy2 23 16 00.6756811155 +25 33 24.081139422   15.0       ~ 205 0
147 SDSS J232231.62+013927.8 G 23 22 31.6234184347 +01 39 28.191471245           ~ 22 0
148 IRAS 23199+0122 PaG 23 22 31.764 +01 39 28.12           ~ 25 0
149 IRAS 23233+2817 Sy2 23 25 49.4068081702 +28 34 21.273807553           ~ 41 1
150 IRAS 23233+0946 LIN 23 25 56.1378291192 +10 02 49.715916252           ~ 61 0
151 2MASS J23351192+2930002 LIN 23 35 11.92032 +29 30 00.2124           ~ 56 0
152 LEDA 90429 SyG 23 39 01.26960 +36 21 08.5896   16.17       ~ 232 1

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