Most light from meteors comes from
spectral lines emitted by the elements they contain, so the impacts may be easiest to see though filters which isolate those lines.
That was consistent with a quasar, but dust blocked the definitive quasar signature of
spectral lines emitted by gas near the black hole.
Based on the wavelengths of
spectral lines emitted by the luminous gas surrounding the black hole, the object is traveling at a speed of about 7.5 million kilometers per hour — a rate that would carry it from Earth to the moon in about 3 minutes.
The metallicity of the gases in the protocluster galaxies was studied using multiple
spectral lines emitted from them.
They detected
a spectral line emitted by neutral helium gas at a wavelength of 1083 nanometres.
Not exact matches
Indeed, its Lyman - alpha spectrum, i.e. one of the
spectral lines of hydrogen it
emits, is much narrower and stronger than that of most galaxies, therefore confirming her theoretical predictions.
Yet so far, star formation historians have mostly relied on other indicators to write their histories: light at a particular frequency that is typically
emitted when giant clouds collapse, heating up in the process and radiating away that heat in the form of specific
spectral lines.
If the atoms are excited, they
emit these same wavelengths, hence one can determine precisely which
spectral lines belong to which element.
This is due to the fact that most visual light is
emitted in one
spectral line, the green 5007 Angstrom forbidden
line of doubly ionized oxygen, [O III](see our Planetary Nebulae page).
Actually, as for almost all planetary nebulae, most of the visible light is even
emitted in one
spectral line only, in the green light at 5007 Angstrom (see our planetary nebula description)!
Starting with the surface, each layer attenuates the BB spectrum with the ghg
lines and will also
emit at the ghg
spectral line wavelengths but with a lower power level if the layer temperature is less.