![]() |
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