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Avedisova star formation regions in sector 30°-20°

This page lists Avedisova star formation regions in the sector with galactic longitude 30°-20° (between galactic latitude -5° and +5°) that contain objects that have at least one bibliographic reference in the SIMBAD database. The regions can be sorted in the order of regions containing objects with the most references or in the order of regions with the most components. The location is linked to a page summarising the data on the star formation region and the object name is linked to the SIMBAD page for that object. Each line also lists the SIMBAD suggested type for that object as well as the number of bibliographic references.

SIMBAD cross reference and type information is not always accurate, so this information should be treated cautiously. It is best to read the bibliographic references for the object to get the latest and most accurate information.

Sort by [Maximum number of SIMBAD references | Number of components]

Region Components Most referenced object Type Object references
29.91-0.05 [20] [WHR97] 18434-0242 HII [201]
26.81+3.54 [7] V* NZ Ser Em* [160]
28.41-1.16 [7] HD 173764 SB [147]
25.65+1.05 [3] [WHR97] 18316-0602 HII [107]
26.35+1.83 [12] LBN 84 HII [99]
25.01+2.10 [3] V* V431 Sct V* [94]
22.95-0.32 [16] SNR G023.3-00.3 SNR [65]
22.76-0.25 [8] SNR G023.3-00.3 SNR [65]
23.26-0.29 [9] SNR G023.3-00.3 SNR [65]
25.38-0.19 [11] V* EW Sct PulsV* [65]
21.82-0.48 [3] PN G021.8-00.4 PN [63]
28.96+3.54 [20] LBN 90 HII [62]
23.96+0.15 [11] [WWB83] G023.96+0.15 HII [56]
24.80+0.10 [16] W 42 HII [52]
25.54+0.20 [4] SNR G025.5+00.2 HII [43]
28.29-0.38 [13] [WHR97] 18416-0420 HII [34]
28.20-0.05 [9] [WHR97] 18403-0417 HII [32]
20.07-0.14 [9] GAL 020.08-00.14 HII [29]
29.42-4.78 [5] LDN 549 DkNeb [27]
27.17-0.08 [4] GPSR5 27.186-0.081 HII [25]
23.40-0.22 [14] [WHR97] 18319-0834 HII [24]
24.47+0.49 [9] [WBH98] 18314-0720 HII [23]
22.40+0.10 [7] GAL 022.357+00.066 HII [22]
28.82-0.23 [9] [WHR97] 18421-0348 HII [21]
24.40-0.19 [3] IRAS 18337-0743 IR [20]
26.60-0.02 [3] WFS 34 HII [20]
23.71+0.18 [10] [WHR97] 18311-0809 HII [20]
23.46+0.07 [7] [WHR97] 18310-0825 HII [20]
21.87+0.01 [8] [WHR97] 18282-0951 HII [18]
24.68-0.15 [10] [WWB83] G024.68-0.16 HII [18]
23.26+0.07 [4] IRAS 18306-0835 IR [18]
27.28+0.15 [15] SNR G027.3+00.1 SNR [18]
21.99+0.03 [5] [SHK2000] 18282-0951 Maser [17]
28.89+0.06 [7] MSX6C G028.8621+00.0657 Region [17]
23.71-0.20 [5] GAL 023.707-00.198 HII [17]
25.41+0.11 [4] IRAS 18345-0641 IR [16]
28.60-0.36 [5] IRAS 18421-0404 YSO [16]
23.20+0.00 [5] IRAS 18308-0841 IR [15]
29.48-0.18 [2] IRAS 18431-0312 IR [15]
27.22-3.45 [3] LDN 518 DkNeb [15]
21.56-0.03 [2] Mol 59 Radio [15]
21.35-0.63 [8] RAFGL 5499 YSO [15]
24.69+0.23 [3] OH 24.69 +0.24 AGB* [15]
29.16-4.82 [5] LDN 542 DkNeb [15]
25.70+0.03 [12] [WHR97] 18353-0628 HII [15]
23.88+4.21 [6] LDN 466 DkNeb [14]
26.52+0.41 [8] IRAS 18355-0532 IR [14]
26.64-4.03 [3] [CB88] 161 DkNeb [13]
25.77+0.21 [5] IRAS 18348-0616 IR [13]
28.27+0.00 [3] RFS 455 Radio [13]
22.69-0.04 [12] LDN 443 DkNeb [13]
29.10-0.70 [8] LBN 91 HII [13]
22.81+0.08 [9] LDN 443 DkNeb [13]
25.79-0.14 [4] [WHR97] 18361-0627 HII [13]
22.73-0.02 [3] LDN 443 DkNeb [13]
24.50-0.04 [7] IRAS 18334-0733 IR [12]
23.45+1.55 [4] IRAS 18258-0737 IR [12]
28.69+0.05 [3] IRAS 18408-0348 HII [12]
25.16+0.08 [4] IRAS 18342-0655 IR [11]
29.88-0.82 [2] IRAS 18460-0307 IR [11]
22.76-0.48 [6] IRAS 18317-0918 YSO [11]
24.72+0.70 [2] V* V481 Sct Be* [11]
28.40+0.07 [2] IRAS 18402-0403 IR [10]
28.80+0.17 [8] IRAS 18406-0338 IR [10]
23.87-0.12 [9] IRAS 18324-0809 IR [10]
28.60+0.02 [6] 2MASS J18432852-0350193 YSO [10]
27.91-0.02 [4] Mol 68 Radio [10]
29.41-1.58 [2] LDN 547 DkNeb [10]
29.21-4.73 [5] LDN 544 DkNeb [9]
26.51+0.28 [2] IRAS 18360-0537 IR [9]
20.99+0.09 [11] IRAS 18263-1036 IR [9]
25.49-0.29 [3] OH 25.50 -0.29 AGB* [9]
26.61-0.21 [4] IRAS 18379-0546 IR [9]
28.48-1.78 [5] LDN 530 DkNeb [9]
25.46-0.21 [3] IRAS 18358-0647 HII [9]
26.61-3.98 [6] LDN 509 DkNeb [9]
25.30+0.21 [6] LBN 82 HII [8]
24.12+0.12 [5] IRAS 18321-0748 IR [8]
29.14-0.15 [5] Mol 70 Radio [8]
26.65+0.02 [4] IRAS 18372-0537 IR [7]
26.30+0.07 [2] Mol 66 Radio [7]
24.74-0.21 [4] GAL 024.74-00.2 HII [7]
23.24-0.11 [4] IRAS 18312-0842 IR [7]
24.46-0.25 [3] IRAS 18340-0738 IR [7]
22.29+4.96 [6] LDN 438 DkNeb [7]
27.98+0.08 [4] IRAS 18394-0425 IR [7]
22.14+4.73 [2] LDN 436 DkNeb [7]
23.81+0.39 [2] IRAS 18305-0758 IR [7]
20.50+0.82 [5] LDN 416 DkNeb [7]
23.58+0.05 [2] IRAS 18314-0820 IR [6]
24.54+0.31 [2] IRAS 18322-0721 IR [6]
28.88-0.02 [2] IRAS 18414-0339 IR [6]
28.32+1.24 [3] [CF95] 35 Maser [6]
21.20-0.89 [3] IRAS 18302-1052 IR [6]
21.39-0.25 [3] IRAS 18282-1024 IR [6]
20.24+0.84 [5] LDN 414 DkNeb [6]
23.13+0.55 [4] LBN 79 HII [6]
29.81+2.22 [3] IRAS 18352-0148 IR [6]
29.22-2.85 [3] [CB88] 164 DkNeb [6]
20.29-1.14 [2] LBN 73 HII [5]
29.75-3.75 [3] LDN 556 DkNeb [5]
27.79-0.27 [2] IRAS 18403-0445 IR [5]
23.37+0.45 [3] IRAS 18295-0819 IR [5]
26.89-3.54 [5] LDN 514 DkNeb [5]
20.06-0.06 [4] LDN 411 DkNeb [5]
24.15-0.01 [2] IRAS 18326-0751 IR [5]
25.31+0.53 [3] IRAS 18328-0634 IR [5]
20.24+0.07 [5] IRAS 18249-1116 IR [5]
23.99-0.09 [3] IRAS 18326-0802 IR [5]
25.28-0.32 [4] IRAS 18358-0659 IR [5]
23.82+0.23 [4] IRAS 18311-0802 IR [5]
24.40+0.07 [6] IRAS 18328-0735 IR [5]
24.33+0.14 [4] IRAS 18324-0737 IR [5]
26.10-0.07 [9] IRAS 18365-0609 IR [5]
22.89+0.68 [2] LBN 78 HII [5]
23.39+0.19 [2] IRAS 18305-0826 IR [5]
27.28-0.17 [7] IRAS 18391-0504 IR [4]
21.60-0.16 [4] IRAS 18283-1011 IR [4]
28.12-1.76 [7] [CB88] 156 DkNeb [4]
23.89+0.07 [5] IRAS 18319-0802 IR [4]
29.89+1.20 [2] LDN 555 DkNeb [4]
24.52-0.28 [4] LBN 80 HII [4]
27.86-0.24 [2] IRAS 18403-0440 IR [4]
23.16-0.38 [3] IRAS 18321-0854 IR [4]
23.42-0.39 [3] IRAS 18326-0840 IR [4]
22.95+0.04 [2] IRAS 18301-0853 IR [4]
28.64+0.19 [4] RFS 465 Radio [4]
29.30-3.36 [4] LDN 545 DkNeb [4]
26.26+0.28 [2] IRAS 18355-0550 IR [4]
25.39+0.55 [4] IRAS 18329-0629 IR [4]
20.90+0.83 [4] [CB88] 140 DkNeb [3]
25.28-0.14 [7] NSV 11126 V* [3]
21.36-0.18 [4] IRAS 18279-1024 IR [3]
29.23-2.78 [3] LDN 561 DkNeb [3]
22.04+0.22 [2] IRAS 18278-0936 IR [3]
29.47-2.98 [2] [CB88] 165 DkNeb [3]
26.32-0.01 [3] IRAS 18367-0556 IR [3]
29.41-3.52 [2] LDN 551 DkNeb [3]
20.72-0.11 [13] IRAS 18264-1052 IR [3]
22.43-0.23 [4] IRAS 18302-0928 IR [3]
28.59+0.14 [3] IRAS 18403-0351 IR [2]
26.82-3.95 [2] [CB88] 162 MolCld [2]
24.22-0.05 [8] IRAS 18328-0748 IR [2]
23.65-0.25 [3] IRAS 18325-0824 IR [2]
26.72+0.17 [4] IRAS 18367-0529 IR [2]
28.43+0.00 [3] IRAS 18405-0402 IR [2]
29.32-4.73 [2] [CB88] 172 MolCld [2]
28.31-0.02 [3] IRAS 18405-0410 IR [2]
25.38-0.34 [5] IRAS 18361-0655 IR [2]
27.12-3.51 [2] [CB88] 159 MolCld [2]
28.16+0.33 [4] IRAS 18388-0409 IR [2]
27.80+0.04 [2] IRAS 18392-0436 IR [2]
29.77+0.22 [3] IRAS 18422-0246 IR [2]
28.00-0.03 [2] IRAS 18398-0426 IR [1]
29.21-0.05 [3] IRAS 18423-0323 IR [1]
27.94+0.20 [4] IRAS 18389-0424 IR [1]
27.65-0.37 [3] IRAS 18404-0455 IR [1]
23.84+0.11 [3] IRAS 18315-0804 IR [1]
21.92-0.39 [4] IRAS 18294-0959 IR [1]
27.13+0.02 [4] IRAS 18382-0510 IR [1]
20.96-0.07 [3] IRAS 18268-1042 IR [1]
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Acknowledgement: based on the Catalog of Star-Forming Regions in the Galaxy ( Avedisova, V. S., Astronomy Reports, Volume 46, Issue 3, March 2002, pp.193-205 [2002ARep...46..193A]). The complete catalog can be accessed here: V/112/.

For more information, read The Avedisova catalog: A real Hitchhiker's Guide to the Galaxy?