| Emission nebula | |
|---|---|
 Thor’s Helmet Nebula imaged on the occasion ofESO’s 50th Anniversary. | |
| Observation data:J2000epoch | |
| Right ascension | 07h 18m 30s[1] |
| Declination | −13° 13.8′ ″[1] |
| Distance | 11,960[2] ly |
| Constellation | Canis Major |
| Notable features | HII (ionized) region |
| Designations | GUM 4, LBN 227.66-00.09, SH 2-298, GRS 227.80 -00.20, LBN 1041, RCW 5[1] |
| See also:Lists of nebulae | |
NGC 2359 (also known asThor's Helmet) is anemission nebula[3] in the constellationCanis Major. The nebula is approximately 3,670parsecs (11.96 thousand light years) away and 30 light-years in size. The central star is theWolf-Rayet starWR7, an extremely hot star thought to be in a brief pre-supernova stage of evolution. It is similar in nature to theBubble Nebula, but interactions with a nearby large molecular cloud are thought to have contributed to the more complex shape and curved bow-shock structure of Thor's Helmet.
It is also catalogued asSharpless 2-298 andGum 4.[4]
The nebula has an overall bubble shape, but with complex filamentary structures. The nebula contains several hundred solar masses of ionised material, plus several thousand more of unionised gas. It is largely interstellar material swept up by winds from the central star, although some material does appear to be enriched with the products of fusion and is likely to come directly from the star.[5] The expansion rate of different portions of the nebula varies from 10 km/s to at least 30 km/s, leading to age estimates of 78,500 - 236,000 years. The nebula has been studied at radio and x-ray wavelengths, but it is still unclear whether it was produced at the class O main sequence stage of development, as ared supergiant,luminous blue variable, or mainly as a Wolf-Rayet star.[2]
NGC 2361 is a bright knot of nebulosity on one edge of the central ring of NGC 2359.
