Avedisova star formation regions in sector 10°-0°

This page lists Avedisova star formation regions in the sector with galactic longitude 10°-0° (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
0.53-0.06 [46] NAME SAGITTARIUS A Radio [755]
0.64-0.05 [120] NAME SAGITTARIUS A Radio [755]
1.13-0.11 [28] NAME SAGITTARIUS A Radio [755]
0.07+0.01 [4] NAME SAGITTARIUS A Radio [755]
6.00-1.20 [67] M 8 HII [378]
7.24+1.49 [2] HD 163296 pMS* [265]
6.99-0.17 [8] M 20 HII [211]
0.18-0.05 [30] NAME QUINTUPLET CLUSTER Cl* [182]
5.89-0.44 [25] [WHR97] 17574-2403 HII [157]
9.62+0.19 [19] [WHR97] 18032-2032 HII [129]
0.33-0.19 [7] ESO 455-39 HII [74]
6.57-1.46 [18] V* V3903 Sgr V* [72]
2.32+1.39 [3] SNR G002.4+01.4 HII [47]
8.67-0.36 [15] [WHR97] 18032-2137 HII [43]
0.50-0.75 [47] [WHR97] 17470-2853 HII [39]
7.47+0.06 [12] [WWB83] G007.47+0.06 HII [33]
0.01-0.55 [9] IRAS 17441-2910 IR [27]
5.48-0.24 [12] [WHR97] 17559-2420 HII [26]
8.97+0.68 [6] LDN 262 DkNeb [24]
8.14+0.23 [12] [WHR97] 17599-2148 HII [23]
6.56-0.09 [14] [WHR97] 17577-2320 HII [20]
0.00+0.19 [10] MGM 1 YSO [19]
0.06-0.07 [8] V* V4535 Sgr Mira [18]
2.85-2.75 [5] LDN 93 DkNeb [18]
0.38+0.02 [7] [WHR97] 17432-2835 HII [16]
5.63+0.23 [5] GAL 005.63+00.24 YSO [15]
6.68-0.25 [9] IRAS 17589-2312 IR [13]
2.61+0.13 [3] [WHR97] 17480-2636 HII [13]
0.52+0.18 [12] IRAS 17430-2822 IR [12]
8.15-1.73 [14] SCHB 305 Maser [12]
0.04+0.02 [6] V* V4922 Sgr V* [12]
4.39+0.10 [9] IRAS 17522-2504 YSO [12]
9.70-0.85 [10] IRAS 18073-2046 YSO [12]
3.88-1.03 [3] [TRC83] 20 HH [11]
8.86-0.33 [6] IRAS 18035-2126 YSO [11]
4.83+0.23 [2] IRAS 17527-2439 HII [11]
0.22-0.01 [4] [WHR97] 17430-2844 HII [10]
0.13-0.55 [6] LBN 2 HII [10]
8.72-0.51 [10] LBN 38 HII [9]
0.33-0.02 [5] IRAS 17433-2838 IR [9]
0.83+0.19 [6] [WHR97] 17436-2807 HII [9]
9.41-0.11 [2] [MHS2002] 177 OH/IR [9]
0.10-0.17 [5] IRAS 17432-2855 IR [9]
8.36-0.30 [4] IRAS 18026-2153 YSO [9]
8.83-0.03 [2] IRAS 18024-2119 IR [8]
2.26+0.23 [7] IRAS 17469-2649 IR [8]
9.02+0.44 [3] PN G009.0+00.4 PN [8]
0.06-0.21 [3] IRAS 17434-2858 IR [8]
1.32+0.10 [3] IRAS 17450-2742 IR [8]
7.60+4.69 [2] LDN 233 DkNeb [8]
4.00+0.33 [4] IRAS 17504-2519 IR [8]
7.55+4.26 [9] LDN 235 DkNeb [8]
2.14+0.01 [3] IRAS 17474-2704 IR [8]
1.33+0.05 [2] IRAS 17450-2742 IR [8]
4.29+0.55 [3] LBN 14 HII [8]
6.37-0.05 [3] IRAS 17571-2328 IR [8]
3.27-0.09 [7] IRAS 17505-2605 IR [8]
0.00-0.18 [2] IRAS 17430-2900 IR [7]
5.19-0.28 [5] IRAS 17555-2436 IR [7]
2.96-0.05 [2] IRAS 17495-2624 IR [7]
0.94-0.08 [3] IRAS 17450-2807 IR [7]
3.43-0.34 [3] IRAS 17517-2609 HII [7]
7.27+0.18 [3] IRAS 17582-2234 IR [6]
7.38+4.10 [3] [CB88] 98 MolCld [6]
2.92-0.01 [3] IRAS 17491-2625 IR [6]
0.48+0.07 [2] IRAS 17433-2828 IR [6]
7.80-0.62 [3] IRAS 18024-2231 IR [6]
4.68+0.28 [3] IRAS 17522-2446 IR [5]
6.47+4.20 [2] PN PM 1-175 post-AGB* [5]
6.15-0.64 [4] IRAS 17588-2358 IR [5]
9.97-0.74 [2] IRAS 18075-2040 IR [5]
0.59-0.06 [10] IRAS 17440-2825 IR [5]
2.53+0.25 [3] IRAS 17474-2637 IR [5]
3.93-0.09 [3] IRAS 17520-2536 IR [5]
8.36-2.13 [5] IRAS 18092-2244 IR [4]
7.65+0.18 [3] 2MASS J18020471-2216186 PN? [4]
8.14-0.03 [3] IRAS 18009-2155 IR [4]
8.53-0.29 [6] IRAS 18026-2145 IR [4]
7.19+0.10 [2] IRAS 17584-2242 IR [4]
5.05-0.19 [3] IRAS 17548-2441 IR [4]
8.42-2.06 [3] [CB88] 114 MolCld [4]
5.06+0.24 [4] IRAS 17531-2426 IR [4]
2.30+3.40 [2] LDN 74 DkNeb [4]
1.98-1.15 [9] IRAS 17515-2747 IR [4]
7.04+0.18 [3] IRAS 17578-2246 IR [4]
6.18+0.56 [3] SH 2-26 HII [4]
3.53+3.64 [2] LDN 114 DkNeb [3]
8.94-0.62 [2] IRAS 18048-2131 IR [3]
2.40+0.07 [3] IRAS 17478-2649 IR [3]
6.55-0.58 [7] BFS 1 HII [3]
4.19-0.05 [3] IRAS 17523-2521 IR [3]
2.59-3.43 [4] [CB88] 109 MolCld [3]
8.38-0.63 [3] IRAS 18036-2201 IR [3]
0.11-0.08 [4] IRAS 17430-2851 IR [3]
3.72+0.02 [3] IRAS 17510-2543 IR [3]
3.43+2.10 [1] RCW 143 HII [2]
2.69+0.14 [3] IRAS 17482-2633 IR [2]
8.00-0.18 [4] IRAS 18011-2206 IR [2]
0.70-0.06 [3] IRAS 17443-2821 IR [2]
1.01-0.24 [5] IRAS 17457-2811 IR [2]
8.48-1.03 [2] IRAS 18052-2205 IR [1]
1.49-0.20 [3] IRAS 17467-2745 IR [1]
4.57-0.16 [4] IRAS 17535-2504 IR [1]
1.13+0.81 [3] IRAS 17420-2731 IR [1]
1.39+0.00 [3] IRAS 17457-2743 IR [1]
9.40+0.15 [3] IRAS 18029-2045 IR [1]

Sector navigation

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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?