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Query : 2004ApJS..154..553S |
2004ApJS..154..553S - Astrophys. J., Suppl. Ser., 154, 553-578 (2004/October-0)
Resolution of distance ambiguities of inner galaxy massive star formation regions. II.
SEWILO M., WATSON C., ARAYA E., CHURCHWELL E., HOFNER P. and KURTZ S.
Abstract (from CDS):
We examined the projected location of H II regions whose distance ambiguities have been resolved (in this work and other similar studies) in the Galactic plane and in a longitude-velocity diagram for a recognizable spiral arm pattern. Although the highest density of points in the position-position plot approximately follows the spiral arms proposed by Taylor & Cordes, the dispersion is still about as large as the separation between their proposed arms. The longitude-velocity plot shows an increase in the density of sources at the points where the spiral arm loci proposed by Taylor & Cordes are approaching the locus of tangent point velocities and a lower density between the arm loci. However, it is not possible to trace spiral arms over significant segments of Galactic longitude in the longitude-velocity plot. We conclude that a very large number of H II regions in combination with more sophisticated Galactic rotation models will be required to obtain a more continuous spiral pattern from kinematic studies of H II regions than from fully sampled surveys of H I or CO.
Abstract Copyright: ∼
Journal keyword(s): Galaxy: Disk - ISM: H II Regions - ISM: Molecules - Radio Lines: ISM - Stars: Formation
VizieR on-line data: <Available at CDS (J/ApJS/154/553): table1.dat table2.dat table3.dat table4.dat table5.dat table7.dat>
Nomenclature: Table 5: [SWA2004] GLL.ll+B.bb MC N, [SWA2004] GLL.lll+B.bbb MC N, N=249.
Simbad objects: 79
Number of rows : 79 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | [CAB2011] G340.06-0.23 | HII | 16 48 11.9 | -45 21 35 | ~ | 13 | 1 | |||||
2 | IRAS 17008-4040 | HII | 17 04 20.5 | -40 44 26 | ~ | 29 | 0 | |||||
3 | IRAS 17009-4042 | HII | 17 04 29.5 | -40 46 27 | ~ | 31 | 0 | |||||
4 | IRAS 17016-4124 | SFR | 17 05 11.160 | -41 29 06.00 | ~ | 60 | 0 | |||||
5 | IRAS 17059-4132 | HII | 17 09 31.3 | -41 35 56 | ~ | 28 | 0 | |||||
6 | SH 2-4 | HII | 17 18 23.9 | -39 19 10 | ~ | 84 | 4 | |||||
7 | IRAS 17178-3742 | HII | 17 21 13.3 | -37 45 18 | ~ | 10 | 0 | |||||
8 | NAME Galactic Center | reg | 17 45 39.60213 | -29 00 22.0000 | ~ | 14417 | 0 | |||||
9 | GAL 010.46+00.03 | HII | 18 08 35.5 | -19 52 09 | ~ | 52 | 0 | |||||
10 | GAL 010.30-00.15 | HII | 18 08 56.11 | -20 05 53.8 | ~ | 82 | 0 | |||||
11 | GAL 010.15-00.34 | HII | 18 09 21.5680 | -20 19 27.720 | ~ | 74 | 0 | |||||
12 | RAFGL 2078 | HII | 18 09 25.9 | -20 19 25 | ~ | 80 | 1 | |||||
13 | CORNISH G010.9584+00.0221 | Y*O | 18 09 39.37824 | -19 26 27.9132 | ~ | 26 | 0 | |||||
14 | W 31 | SFR | 18 10 28.6 | -19 55 51 | ~ | 261 | 0 | |||||
15 | AGAL G012.418+00.506 | cor | 18 10 51.09792 | -17 55 49.6272 | ~ | 66 | 0 | |||||
16 | IRAS 18085-1931 | Y*O | 18 11 31.98 | -19 30 41.7 | ~ | 34 | 0 | |||||
17 | HD 312787 | Em* | 18 11 33.1411451856 | -19 30 31.604296500 | 11.35 | 10.81 | 10.71 | F8 | 21 | 0 | ||
18 | GAL 012.89+00.49 | HII | 18 11 51.3 | -17 31 29 | ~ | 184 | 0 | |||||
19 | OH 012.03-00.04 | Y*O | 18 12 01.8400 | -18 31 55.800 | ~ | 82 | 0 | |||||
20 | IRAS 18092-1742 | HII | 18 12 12.2 | -17 41 55 | ~ | 19 | 0 | |||||
21 | IRAS 18102-1800 | HII | 18 13 12.2 | -17 59 35 | ~ | 23 | 0 | |||||
22 | IRAS 18102-1757 | IR | 18 13 13.3 | -17 56 13 | ~ | 6 | 0 | |||||
23 | CORNISH G011.9368-00.6158 | HII | 18 14 01.0 | -18 53 23 | ~ | 82 | 1 | |||||
24 | GAL 013.875+00.28 | HII | 18 14 35.2 | -16 45 21 | ~ | 92 | 0 | |||||
25 | W 33a | Y*O | 18 14 39.56547 | -17 52 02.2260 | ~ | 698 | 0 | |||||
26 | IRAS 18117-1738 | IR | 18 14 41.3 | -17 37 04 | ~ | 9 | 0 | |||||
27 | IRAS 18153-1651 | IR | 18 18 16.0 | -16 50 39 | ~ | 21 | 0 | |||||
28 | GAL 014.33-00.64 | HII | 18 18 53.5 | -16 47 39 | ~ | 65 | 0 | |||||
29 | IRAS 18161-1626 | IR | 18 19 04.2 | -16 25 14 | ~ | 4 | 0 | |||||
30 | EGO G016.59-0.05 | HII | 18 21 07.9 | -14 31 53 | ~ | 117 | 0 | |||||
31 | OH 016.59-00.05 | Mas | 18 21 09.0840 | -14 31 48.556 | ~ | 81 | 0 | |||||
32 | RAFGL 2136 | Y*O | 18 22 26.52888 | -13 30 14.0400 | ~ | 285 | 0 | |||||
33 | GAL 018.46-00.00 | HII | 18 24 36.4 | -12 51 06 | ~ | 12 | 0 | |||||
34 | IRAS 18223-1243 | Y*O | 18 25 10.9307288448 | -12 42 15.754722912 | ~ | 61 | 1 | |||||
35 | GAL 019.36-00.02 | HII | 18 26 24.3 | -12 03 47 | ~ | 31 | 0 | |||||
36 | GAL 019.07-00.28 | HII | 18 26 47.0 | -12 26 32 | ~ | 26 | 0 | |||||
37 | IRAS 18242-1227 | IR | 18 27 06.0 | -12 25 42 | ~ | 7 | 0 | |||||
38 | MMB G019.884-00.534 | cor | 18 29 14.37 | -11 50 23.0 | ~ | 105 | 1 | |||||
39 | [BNM96] 019.605-0.902 | HII | 18 30 02.7 | -12 15 27 | ~ | 16 | 0 | |||||
40 | IRAS 18272-1217 | Y*O | 18 30 02.77248 | -12 15 22.4172 | ~ | 18 | 0 | |||||
41 | GAL 021.87+00.01 | HII | 18 31 02.5 | -09 49 30 | ~ | 19 | 0 | |||||
42 | [HLB98] SEST 167 | Mas | 18 31 44.2 | -09 22 17 | ~ | 8 | 0 | |||||
43 | GAL 022.357+00.066 | HII | 18 31 44.9 | -09 22 09 | ~ | 45 | 0 | |||||
44 | GAL 021.44-00.56 | Y*O | 18 32 16.2 | -10 28 35 | ~ | 15 | 0 | |||||
45 | AGAL G023.264+00.077 | cor | 18 33 24.00 | -08 33 31.0 | ~ | 41 | 0 | |||||
46 | IRAS 18308-0841 | HII | 18 33 32.89 | -08 39 18.5 | ~ | 33 | 0 | |||||
47 | GAL 023.24-00.24 | HII | 18 34 29.9 | -08 43 23 | ~ | 22 | 0 | |||||
48 | GAL 023.44-00.18 | HII | 18 34 43.6 | -08 32 25 | ~ | 52 | 0 | |||||
49 | GAL 023.707-00.198 | HII | 18 35 12.5 | -08 17 46 | ~ | 28 | 0 | |||||
50 | IRAS 18334-0733 | IR | 18 36 11.0 | -07 31 12 | ~ | 12 | 0 | |||||
51 | RAFGL 5515 | HII | 18 36 29.0 | -07 40 33 | ~ | 30 | 0 | |||||
52 | [BNM96] 024.504-0.218 | HII | 18 36 47.124 | -07 35 41.14 | ~ | 7 | 0 | |||||
53 | GAL 024.68-00.16 | bub | 18 36 53 | -07 24.7 | ~ | 29 | 0 | |||||
54 | GAL 024.75-00.20 | HII | 18 37 09.5 | -07 22 28 | ~ | 10 | 0 | |||||
55 | IRAS 18348-0616 | Y*O | 18 37 30.420 | -06 14 14.49 | 17.34 | 16.14 | 14.80 | ~ | 36 | 0 | ||
56 | [JD2012] G025.460-00.215 | HII | 18 38 30.0 | -06 44 30 | ~ | 12 | 0 | |||||
57 | IRAS 18360-0537 | HII | 18 38 40.3 | -05 35 06 | ~ | 23 | 0 | |||||
58 | IRAS 18361-0627 | mul | 18 38 51.7 | -06 25 01 | ~ | 17 | 0 | |||||
59 | GAL 026.60-00.02 | HII | 18 39 55.9 | -05 38 45 | ~ | 32 | 1 | |||||
60 | AGAL G027.184-00.081 | cor | 18 41 13.26 | -05 08 57.9 | ~ | 57 | 0 | |||||
61 | IRAS 18394-0425 | HII | 18 42 06.34 | -04 22 19.6 | ~ | 15 | 0 | |||||
62 | GAL 028.25+00.01 | Rad | 18 42 54.7 | -04 08 36 | ~ | 14 | 0 | |||||
63 | GAL 028.20-00.04 | HII | 18 42 58.08 | -04 14 04.6 | ~ | 59 | 0 | |||||
64 | 2MASS J18432852-0350193 | Y*O | 18 43 28.52 | -03 50 19.4 | ~ | 11 | 0 | |||||
65 | GAL 028.86-00.07 | HII | 18 43 45.8 | -03 35 30 | ~ | 28 | 0 | |||||
66 | GAL 028.60-00.36 | Y*O | 18 44 48.6 | -04 01 26 | ~ | 17 | 0 | |||||
67 | AGAL G030.423+00.466 | cor | 18 45 12.8 | -02 01 12 | ~ | 31 | 0 | |||||
68 | CORNISH G029.9559-00.0168 | Y*O | 18 46 04.18 | -02 39 21.3 | ~ | 365 | 0 | |||||
69 | IRAS 18440-0148 | cor | 18 46 36.56 | -01 45 21.2 | ~ | 59 | 0 | |||||
70 | IRAS 18445-0222 | HII | 18 47 10.6 | -02 19 08 | ~ | 28 | 0 | |||||
71 | ISOGAL-P J184715.8-014710 | Y*O | 18 47 15.733 | -01 47 10.08 | ~ | 33 | 0 | |||||
72 | IRAS 18449-0115 | cor | 18 47 34.27 | -01 12 43.2 | ~ | 388 | 0 | |||||
73 | GAL 031.07+00.05 | HII | 18 47 51.8 | -01 38 04 | ~ | 11 | 0 | |||||
74 | IRAS 18454-0158 | HII | 18 48 01.3 | -01 54 49 | ~ | 15 | 0 | |||||
75 | GAL 037.76-00.20 | HII | 19 00 59.3 | +04 12 06 | ~ | 11 | 0 | |||||
76 | CORNISH G037.8731-00.3996 | HII | 19 01 53.58 | +04 12 51.7 | ~ | 40 | 1 | |||||
77 | GAL 049.20-00.35 | Cl* | 19 23 02.1 | +14 16 40 | ~ | 65 | 0 | |||||
78 | SH 2-88 B | HII | 19 46 48.2 | +25 12 21 | ~ | 158 | 2 | |||||
79 | NGC 7027 | PN | 21 07 01.571952 | +42 14 10.47120 | 10.358 | 8.831 | 10.157 | ~ | 2459 | 1 |
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