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| physical object > natural object > celestial body > nebula > H II region > gaseous nebula |
| gaseous nebula (emission nebula) | ||||
| subject | fact | |||
| gaseous nebula | has catalog gaseous nebula catalog | ![]() |
| has synonym emission nebula | ![]() | |
| has definition 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. | ![]() | |
| is a kind of H II region | ![]() | |
| H II region | has composition ionized hydrogen | ![]() |
| nebula | is a part of gas | ![]() |
| celestial body | has spectra | ![]() |
| physical object | has location or center of gravity | ![]() |
| has angular momentum | ![]() | |
| has mass | ![]() | |
| has velocity | ![]() | |
| has momentum | ![]() | |
| has temperature | ![]() | |
| has volume | ![]() | |
| has extent | ![]() | |
| has material | ![]() |
Kinds of gaseous nebula :
(9 facts) (NGC 2070, Great Looped Nebula, Tarantula Nebula) - A giant H II region, at least 300 pc across - one of the largest known. It is larger and more luminous than any known in the Galaxy. It is the brightest object in the Large Magellanic Cloud at both optical and radio wavelengths, and contains the densest concentration of W-R stars. (The brightest object near the center is a O+ WN star of Mv = - 10.2.) It is characterized by very rapid, disordered, and complex motions.
(3 facts) (NGC 3372)
(5 facts) (IC 4703)
(9 facts) (M 8, NGC 6523) - An emission nebula in Sagittarius 2 kpc distant.
(4 facts)
(2 facts)
(3 facts)
(11 facts) (Swan Nebula, M 17, NGC 6618) - A bright H II region. It is a double radio source.
(13 facts) (M 42) - A large cloud of gas and dust giving birth to young stars in the constellation Orion and visible to the naked eye. It is an HII region 1500 light-years away., An HII region about 500 pc distant, barely visible to the naked eye in the center of Orion's sword. It is undoubtedly a region where stars are being born; young O stars and many T Tauri variables are associated with it, and its members are extreme Population I. Probably no more than 20000 years old. It is also an X-ray source (3U 0527-05 and M42, NGC 1976)., The Orion Nebula, a star-forming region in the constellation Orion.
(3 facts)
(10 facts) (M 20, NGC 6514) - An emission nebula in Sagittarius.
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