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physical object > natural object > celestial body > Messier object > Omega Nebula |
Omega Nebula comparison table |
Subject | has purpose | is part of | is a kind of | has catalog | is an instance of | has synonym | has image | has definition | has distance | has discoverery date | has discoverer | has composition | has Messier number |
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gaseous nebula | gas | H II region | gaseous nebula catalog | emission nebula | An H II region, a supernova remnant, or a planetary nebula. H II regions have an emission-line optical spectrum, and a thermal continuous spectrum declining in intensity as the wavelength increases (from maximum in the ultraviolet) through infrared and radio. Supernova remnants have an emission-line optical spectrum and a nonthermal radio spectrum. Temperatures of planetary nebulae are much higher than those of H II regions. | ionized hydrogen | |||||||
Messier object | originally to catalog all objects which could be confused with a comet | celestial sphere | celestial body | Messier catalog | an object assigned a number by Charles Messier | from Earth | |||||||
Omega Nebula | originally to catalog all objects which could be confused with a comet | gas | gaseous nebula catalog | Messier object | NGC 6618 | A bright H II region. It is a double radio source. | from Earth | 1745 | Philippe Loys de Cheseaux | ionized hydrogen | 17 |
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