VII/216 H-{alpha} emission regions in Southern Milky Way (Rodgers+ 1960)

VII/216/rcw.dat The Catalogue (tables 2 and 3 of the paper) (181 records)

RCW
---
GLON GLAT
deg deg
RA DE
hm dm
MajAxis
arcmin
MinAxis
arcmin
Br
---
IDs
---
Rem
---
1225.0 -00.607 08. - 11 57150150m NGC2327; HS111,113,114;G2,3 *
2223.8 -01.907 02. - 10 27 14 14b IC2177;HS109;G1 R
3224.2 +01.207 14. - 09 18 4 4b HS115
4224.4 +03.207 21.5- 08 30 60 60f
5227.8 -00.207 16.1- 13 09 8 8b NGC2359; HS116; G4 R
6231.6 -04.307 08.0- 18 24 12 10b G5 R
7232.6 +00.907 29.5- 16 51 17 15m (NGC2409?); G6 R
8233.9 -00.107 28.3- 18 27 3 2b
9234.4 -12.206 43. - 24 20 90 30f R
10234.4 -00.207 29.0- 18 54 18 14f
11234.6 -10.006 52. - 23 35 60 20f R
12234.7 +00.907 33.7- 18 42 6 3b G7
13234.8 -00.107 30.1- 19 18 12 10m R
14235.6 -04.107 17.0- 21 50 6 4m (NGC2367) R
15237.5 -07.307 08. - 25 00300300f R
16243.3 +00.607 51.2- 26 15 33 33b (NGC2467); G9 R
17243.5 -01.007 45.4- 27 13 2 2b
18250.3 -02.207 57.2- 33 42 1 1b
19253.8 -00.508 13.5- 35 42 48 40b G10 R
20254.5 +00.008 17.5- 36 00 10 10m NGC2579; G11 R
21257.6 +00.608 28.8- 38 10 1 1b
22258.1 +12.109 13.5- 31 10 45 45m R
23258.5 +01.408 35.0- 38 21 2 1b
24258.7 -01.408 23.6- 40 12 3 2f
25259.2 +01.308 36.9- 39 02 2 1b
26259.7 +02.908 44.6- 38 27 3 3m
27260.1 +00.508 36.5- 40 12100100m G14 R
28260.1 -03.408 19.6- 42 33 2 1b
29260.2 -03.308 20.0- 42 32 2 2b G13
30260.2 -03.108 21.1- 42 29 2 2b G13 R
31260.7 -03.208 22.3- 42 55 3 2b R
32261.6 +00.908 43.0- 41 09 27 27m G15 R
33263.0 +01.408 49.5- 41 54 95 80m G17 R
34264.4 +01.408 54.4- 42 56 2 2b G19
35264.6 +00.108 49.7- 43 55 30 30m G18
36265.2 +01.408 57.5- 43 33 12 6m G20 R
37267.0 +00.108 58.5- 45 45 13 3f Part of NGC2736 R
38268.0 -01.008 57.5- 47 16 40 40m G22,23,24 R
39269.2 -01.109 01.9- 48 12 2 2b
40269.3 -01.409 01.0- 48 27 8 8b G25 R
41270.3 +00.809 14.8- 47 45 8 4m
42274.1 -01.309 22.4- 51 54 9 7b G26 R
43277.2 -03.809 25.5- 55 54 2 2b NGC2899; G27 R
44277.8 -03.609 29.6- 56 05 2 2f
45282.2 -00.110 10.0- 56 09 16 16f
46282.4 -01.310 06.0- 57 15 15 15f
47283.0 -02.710 03.5- 58 42 25 20m
48283.5 -01.010 14.0- 57 36 15 10b NGC3199; G28 R
49284.3 -00.310 22. - 57 27 90 35b (NGC3247); G29 R
50284.3 +00.410 24.5- 56 54 12 12m R
51286.0 +00.510 36.1- 57 42 12 12b R
52287.2 +00.410 43.5- 58 18 15 15b BBW22500; G32 R
53287.4 -00.910 40. - 59 30210210vbNGC3293,3324,IC2599;BBW22500; *
54289.4 -00.610 58. - 60 06210 60m (NGC3503)?(NGC3572)?G34,5,6,7 *
55290.4 -03.010 54.2- 62 45 8 8m R
56291.1 -02.111 03.3- 62 12 2 1m
57291.6 -00.511 12.5- 60 56170 40m NGC3603; G38,a,b R
58292.4 -04.911 04.3- 65 18 7 7m
59293.0 +04.511 35. - 56 40180150m R
60293.7 -01.411 26.5- 62 30 50 50b IC2872; BBW2620; G39,40 R
61294.2 -02.311 28.3- 63 30 15 15b G41 R
62294.8 -01.511 35. - 62 54 80 80b IC2944,8; BBW26201;G42 R
63297.6 +10.312 17. - 52 00250 40f *
64299.4 -00.312 16.7- 62 41 3 2b
65301.0 +01.212 31.5- 61 18 11 6m G43 R
66301.1 +00.912 32.6- 61 39 2 1m G44
67301.2 +00.812 33.0- 61 45 4 4m
68301.7 +01.012 37.3- 61 36 15 15f
69302.2 +00.312 41.5- 62 18 5 3m G45
70302.7 -01.012 45.6- 63 34 1 1b
71302.9 +01.312 47.3- 61 18 4 3b G46
72303.2 +01.612 50.3- 61 00 2 2f
73303.4 +01.412 52.0- 61 12 2 2m
74305.2 +00.013 07.8- 62 33 15 12f R
75306.3 +00.213 16.5- 62 15 18 13m BBW27300; G48a R
76307.2 -03.513 29.8- 65 45 3 2b NGC5189; G47 R
77307.6 -05.013 35.4- 67 10 1 1b
78307.9 +00.213 30.5- 62 00 45 30f BBW27500; G48b R
79308.7 +00.613 36.5- 61 30 9 5m BBW27600; G48c
80309.3 -00.513 43.5- 62 24 21 10m BBW27700; G48d
81310.6 +00.613 51.9- 61 06 1 1m
82311.0 +00.413 55.7- 61 12 5 4b R
83311.9 -00.514 05.0- 61 50 60 50f BBW27901
84312.6 -02.714 16.4- 63 40 1 1m
85313.5 -00.414 17.0- 61 10 25 20f BBW28100 R
86315.0 -02.314 35.5- 62 27 3 3m R
87320.2 +00.815 01.0- 57 19 2 2b
88320.2 +00.515 02.7- 57 36 3 2b
89320.4 -01.015 09.5- 58 46 4 4f
90321.0 +02.215 01.5- 55 46 1 1m *
91321.2 -00.515 12.5- 58 01 11 10f BBW28801 R
92322.2 +00.615 14.5- 56 30 8 5f BBW28900
93322.6 -02.515 29.7- 58 54 2 2m R
94326.2 +00.915 37.0- 54 00 20 20f BBW29400a R
95326.7 +00.815 39.7- 53 47 3 2b BBW29400c
96326.9 -01.015 48.9- 55 06 2 2f R
97327.1 -00.515 47.7- 54 36 6 5m BBW29401
98327.6 -00.815 51.5- 54 30 6 5b BBW29501; G49 R
99328.7 -00.515 58.8- 53 35 4 2b G50
100329.1 +02.015 47.7- 51 22 1 1m R
101331.7 -01.016 12.6- 51 54 2 2b R
102331.9 -01.016 14.0- 51 48 12 8b BBW29902
103332.4 -00.416 13.3- 51 00 5 3b
104332.9 -01.416 20.2- 51 24 20 20m
105332.9 +01.816 06.3- 49 00 45 35b BBW30000; G51
106332.9 -00.616 17.0- 50 48 35 20m R
107336.4 -00.216 29.8- 48 03 8 4b NGC6164,5; G52 R
108336.5 -01.316 35.0- 48 40210120f (NGC6193); BBW30402; G53 R
109339.7 -00.316 43.0- 45 39 2 2b R
110340.9 -00.816 50.0- 45 00 7 3b G54 R
111341.1 -01.016 51.5- 45 00 5 3b G54 R
112341.7 +05.616 27.0- 40 12 2 2b
113342.7 +01.816 45. - 42 00360300m (NGC6231); BBW31100; G55 R
114343.9 -04.717 18. - 45 00330330f R
115344.4 +07.316 29.6- 37 06 4 2m
117345.5 -01.017 06.2- 41 33 2 2b
118347.3 -00.517 10.0- 39 48 2 2m
119347.7 +01.917 01.3- 38 00180145m (NGC6281); BBW31500; G57,a,b; E1R
120348.3 +00.517 09.0- 38 24 6 6b G58; E2 R
121348.4 -01.117 15.5- 39 15 3 2m E5
122348.9 -01.117 17.1- 38 54 2 2m
123349.5 -00.817 17.8- 38 09 75 75f NGC6337; G59; E6 R
124349.6 +01.117 10.4- 37 00 3 2m NGC6302; E3; G60
125350.0 +00.217 15.0- 37 09 8 8f
126350.6 +01.017 13.5- 36 18 16 4m BBW31800a
127351.4 +00.717 17.0- 35 48 50 25b NGC6334; BBW31800b; E7; HS119 *
128351.4 -00.117 20.4- 36 15 10 10f
129351.9 +12.716 34.0- 28 00180180m R
130352.4 +02.117 14.2- 34 06 30 30m E4 R
131353.2 +00.717 22. - 34 18170 55b (NGC6357); BBW32100; HS120; G66 *
132355.4 +00.217 30. - 32 42110 80m (NGC6383); BBW32301; HS121; G67 *
133355.9 +01.517 26.0- 31 36 45 40m BBW32300; E10; G68 R
134358.5 -01.917 46.1- 31 14 60 50m BBW32603; E17; G69 R
135359.0 -00.717 42.4- 30 12 2 2m
136359.0 -03.617 54.4- 31 40 1 1m R
137359.8 -00.217 42.6- 29 18 18 18b BBW32801; E13 R
138000.1 +00.217 41.7- 28 49 8 4m E12 R
139000.1 -00.317 43.8- 29 02 2 2m E14
140000.2 -00.417 44.2- 29 02 12 12f BBW32701; E16 R
141000.4 -00.217 44.0- 28 46 6 4f E15
142000.6 -00.717 46.5- 28 50 2 2b E18
143003.5 +02.117 42.5- 24 54 7 6m Near NGC6432
144004.4 +00.517 50.7- 25 00 85 65f BBW33201; HS123; E19; G71 R
145006.6 +00.117 57. - 23 15 90 35f HS 124; E20; G74a,b
146006.6 -01.518 03. - 24 00120 90b NGC6523(M8), 6559; BBW33402 *
147007.2 -00.217 59.5- 22 54 16 16b NGC6514(M20); HS125; E22; G76 R
148008.2 +00.617 58.5- 21 35 2 2b
149008.7 -00.618 04.0- 21 45120 30m HS129; E24; G77a
150009.3 +00.318 02.1- 20 48 2 2b R
151011.0 -01.818 13.5- 20 25100 35f NGC6526; HS134; E32,33; G77b R
152012.3 +04.317 53.3- 16 19 2 2m R
153012.2 -01.818 16.0- 19 20 60 20f (IC1283,4); BBW33903; HS140; *
154012.7 +02.018 03.0- 17 00 40 30f
155012.9 +00.318 09.3- 17 41 10 10m HS133; E31 R
156013.7 -00.818 15.0- 17 30 50 50f HS136; E34 R
157014.3 +00.118 13.2- 16 36 60 60b (IC4701); BBW34101; HS137; G79 *
158015.2 +03.318 03.5- 14 12 23 23m BBW34201; HS128; E25; G80
159015.3 -01.818 22.0- 16 36 15 15m R
160015.4 -00.818 18.5- 16 00 70 60b NGC6618; (IC4706,7); BBW34202 *
161016.1 -00.318 18.0- 15 09 80 40m HS143
162016.7 -00.518 20.0- 14 40 22 10b BBW34401; HS146; E44; G82 R
163016.9 -02.318 27.1- 15 24 10 9m
164016.9 -01.218 23.0- 14 51 8 6b HS148; E46
165017.0 +00.818 16. - 13 54 90 66b NGC6611; BBW34400; HS142; G83 *
166018.4 -00.318 22.6- 13 09 15 15f HS147; E45 R
167019.0 +01.318 18. - 11 54180 90m (NGC6604); BBW34600; E41; G84,5
168021.3 +02.518 18.0- 09 16 1 1b
169022.0 +00.118 28.2- 09 48 7 7m HS150; E48 R
170022.6 +00.318 28.5- 09 09 7 5f
171023.2 +00.618 28.6- 08 27 5 5m HS151; E49
172024.6 -00.118 33.8- 07 32 7 7f HS155?; E53
173025.4 +00.218 34.0- 06 41 17 17m BBW35201; HS154; E52
174028.8 +03.418 29.2- 02 13 5 4f HS152
175029.1 -00.718 44.2- 03 48 7 5m HS159; E57 R
176030.5 +00.418 42.7- 02 04 8 8m HS158; E56
177031.9 +01.418 41.8- 00 24 12 12m HS156; E55
178036.3 -01.218 59.2+ 02 19 2 2m
179036.4 -01.719 01.2+ 02 09 20 15f
180038.4 +03.518 46.3+ 06 19 1 1b R
181038.8 +02.018 52.3+ 06 00 5 5f
182040.0 -01.319 06.3+ 05 32 3 3m E61

VII/216/notes.dat Notes to individual nebulae (143 records)

RCW
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add
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Text
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1 Horseshoe-shaped bright region 2 deg. in diameter, with 8'x 5'
1 concentration at 07h 08m, -12 deg 12'. Fainter region 150' diameter,
1 centred on 07h 08m, -09 deg 30'.
1*The original publication gave two positions. Here a single position is
1*given and is very crude.
2 Circular, connected to RCW1 by faint emission.
5 Circular region.
6 Contains diffuse outer region.
7 Circuliar region.
9 Part of the Vela-Puppis Nebula?
11 Part of Vela-Puppis?
13 Circular region.
14 Possibly connected with Vela-Puppis. Possible concentration in RCW15.
15 Loop, possibly connected with Vela-Puppis.
16 Circular region.
19 Large area with one bright edge.
20 Surrounded by diffuse emission; could be associated with RCW19.
22 Part of Vela-Puppis?
27 Region showing structure.
30 Two small regions 1' X 1'.
31 Connected with Vela-Puppis?
32 Circular region.
33 Almost circular, with more intense area "comma"-shaped.
36 Group of 3 bright regions-"S"-shaped.
37 Filamentary.
38 Emission region containing four concentrations at: 08h 57m.5,-47deg 16'(6'
38 X 4'); 08h 57m.7, -47 deg 22'(3 X 2); 08h 58m.0, -47deg 08' (9' X 7'); and
38 08h 58m.4, -47 deg 20'(12 X 9).
40 Bright region possibly associated with diffuse surrounding background
40 emission.
42 Circular.
43 Stellar-like.
48 Bright crescent shape.
49 Emission region outlying Eta Carina nebula.
50 Possibly associated with RCW49.
51 Bright knot possibly separated from the main Eta Carinae nebula by
51 obscuration.
52 Bright knot in Eta Carinae nebula separated from main region by absorption.
53 Main irregular Eta Carinae nebula. Boundaries at 10h 28m, -58 deg; 10h 55m,
53 -58 deg 18'; 10h 27m, -60 deg 48'.
53*The original cross identification also included G30,31, and 33, and
53*NGC3372. Editor's note this is the entire Eta Carinae region.
54 Outlying Eta Carina, with concentrations at: 10h 57m.5, -61 deg 00' (40' X
54 20'); 10h 58m.0, -59 deg 20'(70' X 40')(filamentary); 11h 08m.0, -59 deg
54 54'(25 X 25'); 11h 10m.5, -58 deg 30'(25' X 10').
54*The original gave three positions. The single position given here is
54*extremely crude.
55 Circular region,appears to have central star;not part of Eta Carina.
57 Appears abscuration-bounded and contains bright crescent-shaped region 50'
57 X 20'.
59 3 deg diameter loop.
60 Outlying part of Lambda Cen nebula. Contains bright regions centred at: 11h
60 26m.5, -62 deg 21'(21' X 18'); 11h 26.5m.5, -62 deg 42'(15 X 10).
61 Circular region near Lambda Cen nebula.
62 Main Lambda Cen nebula, uneven intensity.
63 Large band of emission.
63*Two positions are given in the original. The position given here is once
63*again very crude.
65 Region has diffuse edges.
74 Crescent-shaped.
75 Diffuse edges.
76 Planetary?
78 Bright central region (10' X 6').
82 Circular.
85 Possibly obscuration bound.
86 Crescent-shaped.
90*The original size is given as 0.5 X 0.5 arcminutes. Here the size is given
90*as 1 X 1 arcminutes to avoid formating problems.
91 Possibly obscuration bound.
93 Like a planetary in appearance.
94 Circular and filamentary.
96 Appears to be surrounding a star.
98 Appears to be distributed about a faint central star.
100 Stellar-like.
101 Stellar-like.
106 Contains two bright areas: 16h 15m.5, -50 deg 51'(20' X 7'); 16h 17 m.0,
106 -50 deg 42'(12 X 12).
107 Bright region near RCW108.
108 Irregular intensity variation with bright region at 16h 36m, -48 deg
108 30'(60' X 60').
109 Stellar-like.
110 Could be connected to RCW 113 by faint emission.
111 Near RCW110, possibly connected.
113 Large loop of ionization in region of fainter emission. Boundries: (16h
113 37m, -41 deg 50') to (16h 58m, -41 deg 30'); and (16h 50', -43 deg 30') to
113 (16h 45m, -39 deg 40').
114 Ring of emission 50' wide.
116 Concentration inside RCW113 (Editors note; not present in table2&3).
116*Not present in table 2 or 3 of original publication. The notes to table 2
116*and 3 from the original said "116 Concentration inside (RCW)113." This
116*was added to the table to provide a complete list of all 182 objects in
116*the RCW.
119 Filamentary, with bright concentration at 16h 57m.4 -38 deg 13' (15' X15').
120 Contains dark central rift.
123 Loop.
127 Faint extensions to 17h 10m, -35 deg 30'. Composed mainly of four bright
127 concentrations.
127*Other cross identifications given in the original are G61,62,63, 64a,b,c.
129 Region contains the star Tau Sco.
130 Appears to be a more concentrated region of a large area of diffuse
130 emission.
131 Concentrations at: 17h 21m.0, -33 deg 58'(30' X30'); 17h 21m.8, -34 deg
131 10'(9' X9'); 17h 23m.1, -34 deg 27'(6' X 6'); 17 23m.9, -34 deg 03'(5' X
131 5').
131*Other cross identifications given in the original are E8.
132 Crescent-shaped bright region with faint extensions to 17h35m,-34deg
132*Other cross identifications given in the original are E11.
133 Almost circular.
134 Circular.
136 Stellar in appearance.
137 Near galactic centre.
138 Diffuse edges.
140 Perhaps connected to RCW141.
144 Circular.
146 Main bright area divided in three, probably by obscuration, with centres:
146 18h 01m.8, -24 deg 12'(100' X 45'); 18h 03m.0, -23 deg 30' (45' X 45'); 18h
146 06m.5, -23 deg 50'(60' X 50').
146*Other cross identifications given in the original: HS126; E23,27, 29,30;
146*G72,75.
147 Almost circular.
150 Stellar in appearance.
151 Band of emission, one side bounded by heavy obscuration.
152 Stellar in appearance.
153 Faint region with bright area [18h 14m.7, -19 deg 40'(19' X 19')] at one
153 end.
153*The original also gave cross identifications as E39; G78.
155 Two concentrations: 18h 08m.9, -17 deg 36'(7' X 7'); 18h 09m.3, -17 deg
155 40'(8' X 5').
156 Possibly local concentration of general diffuse emmission present. Brighter
156 region at 18h 14m.0, -17 deg 18'(40' X 20').
157 Faint extensions to 18h 01m,-14 deg 00(E25); and 18h 14m,-17 deg 00.
157 [Editors note E25 is designation from Sharpless (1953)].
157*The original also gave cross identifications as E35.
159 Surrounded by diffuse emission.
160 Surrounded by diffuse emission 40' wide.
160*The original also gives HS144, 145; E43; G81a,b.
162 Oval-shaped, possible concentration of general diffuse emission present.
165 Appears connected with adjacent regions by diffuse emission.
166 Surrounded by diffuse emission.
165*The original also gives E42.
169 Circular region.
175 Crescent-shaped.
180 Stellar-like.