Astronomy View all facts Glossary Help |
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 :
Next H II region: H II condensation Up: H II region Previous H II region: compact H II region