Name |
Right Ascension (H.xx) |
Declination (D.xx) |
Distance (kpc) |
Comments |
W51 (A&B) |
19.3879 |
14.4242 |
5.40 |
logL Sun (bolometric luminosity) = 6.67; Num RMS Sources = 24 |
NGC3603 |
11.2510 |
-61.2239 |
7.00 |
logL Sun (bolometric luminosity) = 6.61; Num RMS Sources = 4 |
W49A |
19.1715 |
9.0800 |
11.10 |
logL Sun (bolometric luminosity) = 6.56; Num RMS Sources = 10 |
RCW 106 (G333) |
16.3352 |
-50.5762 |
3.60 |
logL Sun (bolometric luminosity) = 6.28; Num RMS Sources = 33 |
G338.398+00.164 |
16.6742 |
-46.3731 |
12.80 |
logL Sun (bolometric luminosity) = 6.21; Num RMS Sources = 14 |
GAL 331.03-00.15 |
16.1653 |
-51.9131 |
9.60 |
logL Sun (bolometric luminosity) = 6.04; Num RMS Sources = 2 |
G305 |
13.2316 |
-62.6745 |
4.00 |
logL Sun (bolometric luminosity) = 5.94; Num RMS Sources = 25 |
G282.0-1.2 |
10.0653 |
-57.4623 |
7.00 |
logL Sun (bolometric luminosity) = 5.93; Num RMS Sources = 11 |
AGAL032.797+00.191 |
18.8414 |
-0.0307 |
12.90 |
logL Sun (bolometric luminosity) = 5.89; Num RMS Sources = 2 |
W47 |
19.0127 |
4.0525 |
9.90 |
logL Sun (bolometric luminosity) = 5.88; Num RMS Sources = 6 |
G029.956-0.017 |
18.7678 |
-2.6560 |
9.10 |
logL Sun (bolometric luminosity) = 5.87; Num RMS Sources = 1 |
RCW42 |
9.4020 |
-52.0071 |
5.50 |
logL Sun (bolometric luminosity) = 5.86; Num RMS Sources = 5 |
AGAL045.121+00.131 |
19.2243 |
10.8864 |
4.40 |
logL Sun (bolometric luminosity) = 5.82; Num RMS Sources = 2 |
W3 |
2.4358 |
62.0122 |
2.00 |
logL Sun (bolometric luminosity) = 5.80; Num RMS Sources = 9 |
W43 |
18.8027 |
-1.6256 |
4.90 |
logL Sun (bolometric luminosity) = 5.73; Num RMS Sources = 23 |
AGAL319.399-00.012 |
15.0536 |
-58.6031 |
11.60 |
logL Sun (bolometric luminosity) = 5.69; Num RMS Sources = 4 |
Far 3-kpc arm (south) |
17.2701 |
-38.2597 |
11.30 |
logL Sun (bolometric luminosity) = 5.67; Num RMS Sources = 8 |
Near 3-kpc tangent |
16.5824 |
-47.5780 |
7.70 |
logL Sun (bolometric luminosity) = 5.56; Num RMS Sources = 10 |
GAL 331.5-00.1 |
16.2049 |
-51.4383 |
4.90 |
logL Sun (bolometric luminosity) = 5.52; Num RMS Sources = 9 |
G010.960+00.017 |
18.1615 |
-19.4414 |
13.80 |
logL Sun (bolometric luminosity) = 5.50; Num RMS Sources = 2 |
RCW116B |
16.9680 |
-40.3321 |
2.40 |
logL Sun (bolometric luminosity) = 5.43; Num RMS Sources = 14 |
NGC7538 |
23.2410 |
61.4855 |
2.60 |
logL Sun (bolometric luminosity) = 5.43; Num RMS Sources = 9 |
Cygnus X |
20.5073 |
40.8527 |
1.40 |
logL Sun (bolometric luminosity) = 5.40; Num RMS Sources = 74 |
Gum50 |
15.9936 |
-53.7643 |
3.00 |
logL Sun (bolometric luminosity) = 5.38; Num RMS Sources = 1 |
GAL336.40-00.23 |
16.5726 |
-48.0443 |
10.50 |
logL Sun (bolometric luminosity) = 5.30; Num RMS Sources = 5 |
G328.3+0.4 |
15.9017 |
-53.1942 |
5.10 |
logL Sun (bolometric luminosity) = 5.29; Num RMS Sources = 1 |
GAL 010.46+00.02 |
18.1439 |
-19.8755 |
11.20 |
logL Sun (bolometric luminosity) = 5.27; Num RMS Sources = 4 |
AGAL020.746-00.092 |
18.4880 |
-10.8712 |
11.80 |
logL Sun (bolometric luminosity) = 5.26; Num RMS Sources = 2 |
G027.3+00.1 (SNR) |
18.6762 |
-4.9660 |
12.60 |
logL Sun (bolometric luminosity) = 5.26; Num RMS Sources = 2 |
W39 |
18.4445 |
-12.6768 |
4.50 |
logL Sun (bolometric luminosity) = 5.26; Num RMS Sources = 4 |
G024.78+00.08 |
18.6038 |
-7.1807 |
7.70 |
logL Sun (bolometric luminosity) = 5.23; Num RMS Sources = 3 |
M17 |
18.3418 |
-16.1109 |
2.00 |
logL Sun (bolometric luminosity) = 5.23; Num RMS Sources = 8 |
G284.00 -01.00 |
10.3366 |
-58.0745 |
4.70 |
logL Sun (bolometric luminosity) = 5.22; Num RMS Sources = 5 |
W33 |
18.2218 |
-17.7443 |
2.40 |
logL Sun (bolometric luminosity) = 5.21; Num RMS Sources = 7 |
GAL336.84+00.05 |
16.5800 |
-47.6010 |
10.90 |
logL Sun (bolometric luminosity) = 5.21; Num RMS Sources = 3 |
AGAL020.081-00.136 |
18.4696 |
-11.4860 |
7.90 |
logL Sun (bolometric luminosity) = 5.17; Num RMS Sources = 2 |
Vul OB1 |
19.7428 |
24.1968 |
2.20 |
logL Sun (bolometric luminosity) = 5.16; Num RMS Sources = 16 |
G52.04+0.55 |
19.4131 |
17.3060 |
9.90 |
logL Sun (bolometric luminosity) = 5.12; Num RMS Sources = 4 |
AGAL023.711+00.171 |
18.5649 |
-8.1216 |
7.70 |
logL Sun (bolometric luminosity) = 5.11; Num RMS Sources = 1 |
GAL 337.9-00.5 |
16.6857 |
-47.1140 |
3.00 |
logL Sun (bolometric luminosity) = 5.10; Num RMS Sources = 1 |
G048.60+0.02 |
19.3422 |
13.9302 |
10.80 |
logL Sun (bolometric luminosity) = 5.10; Num RMS Sources = 4 |
W31-south |
18.1502 |
-20.0856 |
3.60 |
logL Sun (bolometric luminosity) = 5.10; Num RMS Sources = 2 |
AGAL307.616-00.259 |
13.5423 |
-62.7553 |
7.00 |
logL Sun (bolometric luminosity) = 5.09; Num RMS Sources = 3 |
W31-North |
18.1777 |
-19.8391 |
5.00 |
logL Sun (bolometric luminosity) = 5.08; Num RMS Sources = 5 |
AGAL337.406-00.402 |
16.6477 |
-47.4690 |
3.10 |
logL Sun (bolometric luminosity) = 5.03; Num RMS Sources = 4 |
G298.2-0.3 |
12.1668 |
-62.8314 |
4.70 |
logL Sun (bolometric luminosity) = 5.02; Num RMS Sources = 1 |
G347.600+00.211 |
17.1943 |
-39.1398 |
5.90 |
logL Sun (bolometric luminosity) = 5.02; Num RMS Sources = 5 |
GAL 331.35+01.07 |
16.1048 |
-50.7031 |
4.60 |
logL Sun (bolometric luminosity) = 5.01; Num RMS Sources = 3 |
AGAL300.504-00.176 |
12.5012 |
-62.9470 |
8.90 |
logL Sun (bolometric luminosity) = 4.99; Num RMS Sources = 3 |
GAL 338.01-00.12 |
16.6664 |
-46.8504 |
11.40 |
logL Sun (bolometric luminosity) = 4.98; Num RMS Sources = 5 |
S269 |
6.2436 |
13.8264 |
5.30 |
logL Sun (bolometric luminosity) = 4.97; Num RMS Sources = 1 |
RCW121 |
17.3431 |
-38.7964 |
2.80 |
logL Sun (bolometric luminosity) = 4.97; Num RMS Sources = 10 |
Gemini OB1 |
6.1626 |
19.3780 |
2.00 |
logL Sun (bolometric luminosity) = 4.95; Num RMS Sources = 12 |
DR7 |
20.4710 |
40.8871 |
7.30 |
logL Sun (bolometric luminosity) = 4.94; Num RMS Sources = 3 |
GAL 343.36+0.1 |
16.9850 |
-42.6704 |
2.80 |
logL Sun (bolometric luminosity) = 4.94; Num RMS Sources = 6 |
AGAL314.219+00.271 |
14.4203 |
-60.5363 |
5.90 |
logL Sun (bolometric luminosity) = 4.93; Num RMS Sources = 2 |
GRS 319.38-00.03 |
15.0616 |
-58.5856 |
11.40 |
logL Sun (bolometric luminosity) = 4.89; Num RMS Sources = 1 |
S156 |
23.0875 |
60.2099 |
4.30 |
logL Sun (bolometric luminosity) = 4.88; Num RMS Sources = 3 |
AGAL321.379-00.301 |
15.2894 |
-57.8429 |
9.40 |
logL Sun (bolometric luminosity) = 4.85; Num RMS Sources = 3 |
AGAL295.153-00.587 |
11.7248 |
-62.4268 |
9.80 |
logL Sun (bolometric luminosity) = 4.85; Num RMS Sources = 2 |
AGAL338.926+00.554 |
16.6758 |
-45.6963 |
4.20 |
logL Sun (bolometric luminosity) = 4.84; Num RMS Sources = 2 |
G018.20-0.32 |
18.4117 |
-13.2795 |
4.10 |
logL Sun (bolometric luminosity) = 4.83; Num RMS Sources = 3 |
AGAL323.741-00.264 |
15.5291 |
-56.5096 |
3.20 |
logL Sun (bolometric luminosity) = 4.81; Num RMS Sources = 5 |
G345.50+00.35 |
17.0738 |
-40.7568 |
2.00 |
logL Sun (bolometric luminosity) = 4.78; Num RMS Sources = 2 |
S138 |
22.5430 |
58.3943 |
4.60 |
logL Sun (bolometric luminosity) = 4.76; Num RMS Sources = 2 |
GRS 330.88 -00.36 |
16.1726 |
-52.1097 |
3.90 |
logL Sun (bolometric luminosity) = 4.73; Num RMS Sources = 4 |
G316.8-0.1 |
14.7573 |
-59.8208 |
2.70 |
logL Sun (bolometric luminosity) = 4.65; Num RMS Sources = 1 |
AGAL300.969+01.146 |
12.5812 |
-61.6585 |
4.30 |
logL Sun (bolometric luminosity) = 4.63; Num RMS Sources = 1 |
G333.18-00.07 |
16.3313 |
-50.3037 |
5.10 |
logL Sun (bolometric luminosity) = 4.62; Num RMS Sources = 3 |
AGAL340.248-00.374 |
16.8245 |
-45.2998 |
3.70 |
logL Sun (bolometric luminosity) = 4.58; Num RMS Sources = 2 |
AGAL043.179-00.519 |
19.2025 |
8.8678 |
8.20 |
logL Sun (bolometric luminosity) = 4.56; Num RMS Sources = 1 |
G013.25-00.07 |
18.2444 |
-17.4979 |
9.40 |
logL Sun (bolometric luminosity) = 4.55; Num RMS Sources = 3 |
RCW49/Westerlund 2 |
10.4037 |
-57.7981 |
2.80 |
logL Sun (bolometric luminosity) = 4.55; Num RMS Sources = 6 |
G331.28-0.19 |
16.1906 |
-51.7012 |
5.00 |
logL Sun (bolometric luminosity) = 4.54; Num RMS Sources = 1 |
RCW95 |
15.7421 |
-54.0604 |
1.80 |
logL Sun (bolometric luminosity) = 4.51; Num RMS Sources = 6 |
G347.893+00.044 |
17.2192 |
-38.9856 |
3.30 |
logL Sun (bolometric luminosity) = 4.47; Num RMS Sources = 5 |
WB 89-437 |
2.7246 |
62.9527 |
6.00 |
logL Sun (bolometric luminosity) = 4.46; Num RMS Sources = 1 |
G010.84-02.60 |
18.3204 |
-20.7944 |
1.90 |
logL Sun (bolometric luminosity) = 4.45; Num RMS Sources = 2 |
G327.3-0.6 |
15.8838 |
-54.6259 |
3.00 |
logL Sun (bolometric luminosity) = 4.44; Num RMS Sources = 3 |
NGC3372, Carina Nebula |
10.7311 |
-59.5472 |
2.50 |
logL Sun (bolometric luminosity) = 4.42; Num RMS Sources = 8 |
Vela Molecular Ridge |
8.8772 |
-44.7579 |
0.70 |
logL Sun (bolometric luminosity) = 4.41; Num RMS Sources = 34 |
Onsala 1 |
20.1691 |
31.5260 |
2.50 |
logL Sun (bolometric luminosity) = 4.41; Num RMS Sources = 1 |
G338.934-00.067 |
16.7674 |
-45.6288 |
2.80 |
logL Sun (bolometric luminosity) = 4.40; Num RMS Sources = 2 |
Far 3-kpc arm (north) |
18.2006 |
-18.5319 |
11.10 |
logL Sun (bolometric luminosity) = 4.39; Num RMS Sources = 1 |
Auriga OB1 |
5.6695 |
35.7588 |
2.00 |
logL Sun (bolometric luminosity) = 4.37; Num RMS Sources = 6 |
W5 |
2.8786 |
61.2886 |
3.00 |
logL Sun (bolometric luminosity) = 4.36; Num RMS Sources = 5 |
GAL 336.9-00.2 |
16.5984 |
-47.6586 |
4.50 |
logL Sun (bolometric luminosity) = 4.35; Num RMS Sources = 3 |
AGAL331.134-00.484 |
16.2006 |
-52.0242 |
4.00 |
logL Sun (bolometric luminosity) = 4.35; Num RMS Sources = 2 |
AGAL333.017+00.766 |
16.2545 |
-49.8157 |
3.20 |
logL Sun (bolometric luminosity) = 4.34; Num RMS Sources = 2 |
RCW79 |
13.6687 |
-61.7349 |
4.00 |
logL Sun (bolometric luminosity) = 4.27; Num RMS Sources = 6 |
GAL331.517-00.069 |
16.1830 |
-51.8423 |
4.90 |
logL Sun (bolometric luminosity) = 4.27; Num RMS Sources = 1 |
G024.78+00.08? |
18.5975 |
-7.2223 |
7.70 |
logL Sun (bolometric luminosity) = 4.12; Num RMS Sources = 1 |
W42 |
18.6295 |
-6.7020 |
2.70 |
logL Sun (bolometric luminosity) = 4.12; Num RMS Sources = 4 |
AGAL297.472-00.727 |
12.0482 |
-63.0879 |
9.70 |
logL Sun (bolometric luminosity) = 4.12; Num RMS Sources = 2 |
M16 |
18.3139 |
-13.7847 |
2.20 |
logL Sun (bolometric luminosity) = 4.08; Num RMS Sources = 7 |
Gum48d |
13.8159 |
-62.8016 |
3.50 |
logL Sun (bolometric luminosity) = 4.05; Num RMS Sources = 5 |
G338.943+0.604 |
16.6701 |
-45.6928 |
4.00 |
logL Sun (bolometric luminosity) = 4.02; Num RMS Sources = 2 |
AGAL284.734+00.326 |
10.4923 |
-57.4440 |
5.20 |
logL Sun (bolometric luminosity) = 3.95; Num RMS Sources = 1 |
Cep A |
22.8631 |
62.0424 |
0.70 |
logL Sun (bolometric luminosity) = 3.93; Num RMS Sources = 2 |
G338.28+00.53 |
16.6364 |
-46.1950 |
4.10 |
logL Sun (bolometric luminosity) = 3.93; Num RMS Sources = 4 |
NGC3293 |
10.6241 |
-58.5129 |
2.30 |
logL Sun (bolometric luminosity) = 3.92; Num RMS Sources = 3 |
G311.48+0.37 |
14.0623 |
-61.2908 |
3.70 |
logL Sun (bolometric luminosity) = 3.91; Num RMS Sources = 2 |
AGAL337.632-00.079 |
16.6386 |
-47.0811 |
3.80 |
logL Sun (bolometric luminosity) = 3.88; Num RMS Sources = 2 |
GAL335.98+00.19 |
16.5130 |
-48.1813 |
3.70 |
logL Sun (bolometric luminosity) = 3.87; Num RMS Sources = 2 |
Gemini OB1, IRAS 06058+2138 |
6.1483 |
21.6403 |
1.80 |
logL Sun (bolometric luminosity) = 3.86; Num RMS Sources = 1 |
AGAL014.607+00.012 |
18.2837 |
-16.2452 |
2.70 |
logL Sun (bolometric luminosity) = 3.76; Num RMS Sources = 2 |
G014.51-00.55 IRDC Complex |
18.3103 |
-16.8510 |
1.10 |
logL Sun (bolometric luminosity) = 3.72; Num RMS Sources = 5 |
G338.925+0.387 |
16.6882 |
-45.8066 |
2.20 |
logL Sun (bolometric luminosity) = 3.60; Num RMS Sources = 3 |
BFS57 |
6.9873 |
-3.9543 |
1.30 |
logL Sun (bolometric luminosity) = 3.54; Num RMS Sources = 2 |
GAL 338.92-00.09 |
16.7211 |
-46.0949 |
3.30 |
logL Sun (bolometric luminosity) = 3.53; Num RMS Sources = 1 |
Sh 2-187, LBN 630 |
1.3740 |
61.7039 |
0.70 |
logL Sun (bolometric luminosity) = 3.43; Num RMS Sources = 3 |
GAL 343.93-00.64 |
17.0583 |
-42.6308 |
2.80 |
logL Sun (bolometric luminosity) = 3.27; Num RMS Sources = 1 |
N4 Bubble |
18.1497 |
-18.2747 |
2.90 |
logL Sun (bolometric luminosity) = 3.26; Num RMS Sources = 1 |
GAL 340.24+00.48 |
16.7556 |
-44.7966 |
3.80 |
logL Sun (bolometric luminosity) = 3.11; Num RMS Sources = 1 |
IRAS 05137+3919 |
5.2872 |
39.3720 |
2.00 |
logL Sun (bolometric luminosity) = 3.09; Num RMS Sources = 1 |
RCW 82 |
13.9920 |
-61.3922 |
2.90 |
logL Sun (bolometric luminosity) = 3.06; Num RMS Sources = 2 |
NGC3576 |
11.1935 |
-61.3011 |
1.00 |
logL Sun (bolometric luminosity) = 2.59; Num RMS Sources = 1 |
Sun |
0 |
0 |
0 |
|