Uncataloged OIII regions

Objects in this list were detected in [OIII] light. Usually they also can be seen in other wavelengths.

Click the link in the first column to query for images on this site. A detailed description of the table and catalog can be found on the catalog's main page.

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ID
RA
in h m s
DEC
in ° ′ ″
GLON
in °
GLAT
in °

Major
diameter
in ′
Minor
diameter
in ′
Angle
in °


Old
ID


Publication
date
Comment
Images O184.8 6 23 07.0 +28 00 37 184.8435 +6.7360 3.364 K3 2024-06-28 Tiny nebula bright in [OIII] and H-alpha.
Images O190.7 5 56 00.3 +17 57 41 190.6554 -3.5641 10.10 K5 2024-06-28 Small nebula bright in [OIII] and H-alpha. Possible ionization source hot subdwarf KPD 0553+1755: PN candidate.
(KPD 0553+1755) 5 56 02.3 +17 56 13 190.6804 -3.5695 Possible progenitor of O190.7. Distance according to Gaia DR3: about 1900 pc.
Images O200.0 7 41 48.4 +19 56 34 200.0324 +19.7501 1015 181.5 173 K1a, O201.5 2024-06-28 Large (17° x 2.5°) arc with dominant [OIII] emissions
(O200.0a) 7 42 39.7 +21 04 02 199.0072 +20.3643 183.8 120.0 173 K1b, O201.5a 2024-06-28 Part of O200.0 only visible in H-alpha and [SII]
(O200.0b) 7 50 53.0 +12 31 23 208.1575 +18.7661 181.1 43.90 175 O201.5b 2025-05-22 Very faint OIII filament that appear to belong to O200.0
Images O205.0 7 55 18.1 +16 14 54 204.9999 +21.2606 309.9 99.86 167 K1c, O204.0 2024-06-28 Filaments that might belong to Monogem Ring and emit at all three wavelengths
Images O026.2 7 28 43.4 +13 20 51 205.0103 +14.2130 30.23 20.46 133 2025-05-22 Faint halo of the bright center structure O026.2a.
(O026.2a) 19 43 26.9 -13 44 47 26.1932 -17.6294 8.204 2025-05-22 Filled OIII ring. Very faint in H-alpha.
Images O027.9 19 50 45.2 -12 46 00 27.9095 -18.8392 311.6 77.23 83 2025-05-22 OIII filament. Ends are also visible in H-alpha. Probably not related to O026.1.
Images O043.0 19 31 33.2 +6 07 50 43.0091 -6.0504 15.59 7.777 153 2025-05-22 Faint OIII region also visible in H-alpha
Images O043.8 19 03 38.2 +10 42 21 43.8442 +2.1880 10.87 2025-05-22 Faint in [OIII] but clearly visible in H-alpha.
Images O047.3 19 52 24.4 +8 10 20 47.3299 -9.6010 10.18 2025-05-22 Very faint OIII and HII region.
Images O058.9 20 50 57.8 +12 18 37 58.8518 -19.6324 122.2 2025-05-22 OIII region possibly belonging to HII/SII filaments in the same region.
Images O061.2 18 56 18.0 +30 41 41 61.2175 +12.5052 13.93 2025-05-22
Images O074.2 21 08 24.6 +27 50 53 74.2531 -13.2853 48.31 2025-05-22 Faint OIII region with white dwarf GALEX J210824.9+275048 in the center: PN candidate.
(GALEX J210824.9+275048) 21 08 25.0 +27 50 50 74.2532 -13.2868 Possible progenitor of O074.2. Distance according to Gaia DR3: about 500 pc.
Images O077.4 21 02 08.9 +33 02 48 77.3637 -8.8659 68.82 18.23 55 2025-05-22 OIII/SII filament. Probably a part of a SNR.
Images O081.9 21 51 04.0 +28 58 58 81.9365 -19.1879 285.8 2025-05-22 Large OIII region with very nearby hot subdwarf BD+28 4211 in the center: PN candidate.
(BD+28 4211) 21 51 11.0 +28 51 50 81.8728 -19.2934 Possible progenitor of O081.9. Distance according to Gaia DR3: about 110 pc.
Images O084.4 19 26 00.9 +52 50 03 84.4232 +16.4130 74.56 2025-05-22 Faint but large object. Possibly ionized by the hot subdwarf GALEX J192429.7+530554 (not in the center of the OIII region).
(GALEX J192429.7+530554) 19 24 29.6 +53 05 54 84.5819 +16.7279 Possible ionization source of O084.4. Distance according to Gaia DR3: about 780pc.
Images O083.6 19 53 28.3 +49 46 27 83.5565 +11.2135 26.49 8.912 106 2025-05-22 Elongated OIII object also visible in H-alpha.
Images O092.7 22 45 25.9 +29 40 54 92.6838 -25.6878 67.42 44.34 164 2025-05-22 Very faint but visible in [OIII], [SII] and H-alpha.
Images O100.8 20 49 59.7 +64 58 40 100.7540 +13.1219 37.29 2025-05-22 Faint OIII region also visible in [SII]. White dwarf candidate Gaia DR3 2197568743407319552 in center: PN candidate
(Gaia DR3 21975..319552) 20 49 52.8 +64 55 53 100.7087 +13.1035 Gaia DR3 2197568743407319552. Possible progenitor of O100.8. Distance according to Gaia DR3: about 1000pc
Images O102.9 18 30 36.4 +72 12 40 102.9072 +27.3138 37.88 2025-05-22 Very faint OIII region with white dwarf HS 1830+7209 in the center: PN candidate
(HS 1830+7209) 18 30 04.7 +72 11 36 102.8839 +27.3528 Possible progenitor of O102.9. Distance according to Gaia DR3: about 3700 pc.
Images O103.7 20 02 59.6 +71 00 26 103.6866 +20.0102 183.0 2025-05-22 Bright nebula visible in [OIII], [SII], and H-alpha. The bright H-alpha spot near the northern boundary of the OIII region is EGB 10 and is currently classified as a galaxy (2013MNRAS.431....2F), diffuse nebula (1988PASP..100..680H), or possible planetary nebula (1984PASP...96..283E). Due to its position and morphology, EGB 10 may be unrelated to the large structure.
(EGB 10) 20 04 24.0 +71 48 00 104.4993 +20.2529
Images O104.4 15 02 50.6 +66 00 50 104.3887 +46.0993 164.3 2025-05-22 Large and faint OIII ring. Possibly ionized by the white dwarf PG 1501+664: PN candidate.
(PG 1501+664) 15 02 09.6 +66 12 19 104.6518 +46.0095 Possible ionization source of O104.4. Distance according to Gaia DR3: about 460 pc.
Images O106.4 21 48 40.1 +66 58 29 106.4113 +10.1660 74.25 18.25 22 2025-05-22 OIII filament in a region with many HII/SII filaments.
Images O109.4 22 27 39.1 +66 44 08 109.4002 +7.7197 1.887 2025-05-22 Tiny but bright OIII object. Also visible in H-alpha.
(O109.4a) 22 27 39.6 +66 44 23 109.4032 +7.7228 8.514 2020-05-28 There might be a very faint halo around O109.4
Images O109.6 22 14 05.5 +69 01 19 109.5953 +10.3303 116.7 28.69 84 2025-05-22 OIII filament in a region with many HII/SII filaments.
Images O110.1 23 56 19.0 +34 07 56 110.1050 -27.3628 30.18 10.91 103 2025-05-22 Faint OIII arc.
Images O111.7 23 23 00.4 +58 56 14 111.7277 -1.9973 11.05 2025-05-22 OIII region also with faint H-alpha emissions.
Images O111.9 23 40 18.9 +51 53 56 111.9194 -9.4455 21.56 H112.0 2023-02-05 Was H112.0. Much larger in OIII.
Images O119.8 0 41 38.9 +20 10 11 119.8083 -42.6427 40.34 2025-05-22 OIII ring probably ionized by the White Dwarf PG 0038+199: PN candidate.
(PG 0038+199) 0 41 35.3 +20 09 17 119.7882 -42.6569 Likely the ionization source of O119.8. Distance according to Gaia DR3: about 400pc.
Images O138.5 3 08 06.4 +61 25 11 138.5355 +2.7595 44.62 2025-05-22 Faint OIII region hidden within or behind molecular clouds.
Images O141.6 8 23 53.1 +72 59 12 141.5530 +32.5641 21.43 H147.7 2024-10-24 Also very faint [OIII] emissions. Was H147.7.
Images O159.1 4 37 02.9 +44 49 01 159.1663 -1.6016 22.36 16.80 110 2025-05-22 Faint in [OIII], but also some H-alpha emissions. In the center of the OIII region there is the white dwarf Gaia DR3 253119465183909760: PN candidate
(Gaia DR3 25311..909760) 4 37 31.9 +44 48 13 159.2339 -1.5469 Possible ionization source of O159.1. Distance according to Gaia DR3: about 60pc.
Images O163.8 9 56 28.1 +51 45 24 163.7755 +49.1242 36.61 20.35 52 H163.6 2024-10-24 Was H163.6. Larger in [OIII]. Possibly ionized (but not in the center of the OIII region) by the hot subdwarf GD 300.
(GD 300) 9 55 19.5 +51 36 59 164.0681 +49.0044 Gaia DR3 253119465183909760. Possible ionization source of O163.8. Distance according to Gaia DR3: about 590 pc.
Images O166.6 4 14 20.8 +30 23 27 166.6137 -14.7905 2.516 2025-05-22 Tiny object clearly visible in [OIII] and H-alpha.
Images O168.7 5 09 26.8 +37 32 06 168.6561 -1.4900 93.62 H168.8 2022-10-19 Faint [OIII] ring. Possible SNR. Was H168.8.
Images O170.8 10 28 55.9 +45 14 11 170.8107 +56.4258 494.4 170.5 124 H170.2 2024-10-25 Was H170.2. Larger with [OIII] and [SII] emissions. Several white dwarfs in the OIII region.
Images O176.9 5 25 21.8 +29 47 46 176.8927 -3.2509 53.58 2025-05-22 Faint emission nebula visible in [OIII], [SII] and H-alpha. Possibly ionized by HD 35347.
(HD 35347) 5 25 17.8 +29 36 54 177.0351 -3.3641 Possible ionization source of O176.8. Distance according to Gaia DR3: about 1600 pc.
Images O178.2 5 47 20.8 +31 14 15 178.2272 +1.5143 45.37 2025-05-22 Faint OIII region. Also visible in H-alpha.
Images O179.5 6 46 23.0 +36 07 57 179.5078 +14.6564 44.32 2025-05-22 Unstructured nebula only visible in [OIII].
Images O182.3 5 38 27.4 +25 13 05 182.3214 -3.3139 38.07 6.212 140 2025-05-22 Very faint filament which is at least visible on [OIII] and H-alpha
Images O182.8 5 43 31.5 +25 19 03 182.8424 -2.2882 37.71 2025-05-22 Very faint OIII object within SII and HII filaments. Possibly ionized by HD 38010
(HD 38010) 5 43 39.1 +25 26 22 182.7534 -2.2002 2025-05-22 Possible ionization source of .... Distance according to Gaia DR3: about 780 pc
Images O183.7 6 06 16.2 +27 21 15 183.6586 +3.1379 19.34 2025-05-22
Images O187.1 3 48 30.9 +0 46 25 187.0593 -39.1297 27.30 2025-05-22 OIII region probably ionized by White Dwarf KUV 03459+0037: PN candidate.
(KUV 03459+0037) 3 48 31.3 +0 46 16 187.0632 -39.1296 Probably the ionization source of O187.1. Distance according to Gaia DR3: about 390 pc.
Images O190.7 7 16 03.8 +27 03 21 190.7355 +17.0020 65.85 24.44 156 2025-05-22 Faint OIII filament that is also visible in H-alpha.
Images O192.3 6 25 18.8 +19 52 30 192.3238 +3.4296 83.50 2025-05-22 Large OIII region. There are several O stars in that direction, located at different distances, e.g. HD 256725 or HD 44811. It is uncertain whether the much smaller HII structure SH2-253 is related to this object.
(HD 256725) 6 25 01.3 +19 50 56 192.3150 +3.3566 Possible ionization source of O192.3. Distance according to Gaia DR3: about 4500 pc.
(HD 44811) 6 24 38.4 +19 42 16 192.4013 +3.2098 Possible ionization source of O192.3. Distance according to Gaia DR3: about 2000 pc.
Images O204.5 7 36 14.1 +14 44 15 204.4925 +16.4492 37.39 2025-05-22 Faint OIII region which may be ionized by the nearby white dwarf UCAC4 524-042847: PN candidate.
(UCAC4 524-042847) 7 36 07.9 +14 44 51 204.4722 +16.4307 Possible ionization source of O204.5. Distance according to Gaia DR3: about 150 pc.
Images O211.2 7 29 43.5 +6 47 13 211.1837 +11.5859 34.57 22.09 32 2025-05-22 Possibly ionized by the white dwarf Gaia DR3 3141806239596379136.
(Gaia DR3 31418..379136) 7 29 22.2 +6 45 21 211.1722 +11.4935 Gaia DR3 3141806239596379136. Possible ionization source of O211.2. Distance according to Gaia DR3: about 290 pc
Images O220.2 6 02 35.5 -13 59 38 220.2401 -17.0334 73.10 2025-05-22 Very faint but large structure. Possibly ionized by white dwarf UCAC4 381-011163: PN candidate.
(UCAC4 381-011163) 6 02 45.0 -13 51 04 220.1209 -16.9392 Possible ionization source of O220.2. Distance according to Gaia DR3: about 390 pc.

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