hidrogénvonalak
Hidrogénvonalak, also known as hydrogen lines, are specific wavelengths of light emitted or absorbed by hydrogen atoms. These lines are fundamental to astronomy and astrophysics as they provide crucial information about the composition, temperature, and motion of celestial objects.
The most prominent hydrogen lines are part of the Balmer series, which occur in the visible spectrum.
The presence and intensity of these lines in the light from stars, nebulae, and galaxies act as
Beyond the visible spectrum, hydrogen also has lines in the ultraviolet (Lyman series) and infrared (Paschen