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  2. Lyman series - Wikipedia

    en.wikipedia.org/wiki/Lyman_series

    The transitions are named sequentially by Greek letters: from n = 2 to n = 1 is called Lyman-alpha, 3 to 1 is Lyman-beta, 4 to 1 is Lyman-gamma, and so on. The series is named after its discoverer, Theodore Lyman. The greater the difference in the principal quantum numbers, the higher the energy of the electromagnetic emission.

  3. Lyman-alpha - Wikipedia

    en.wikipedia.org/wiki/Lyman-alpha

    Lyman-alpha, typically denoted by Ly-α, is a spectral line of hydrogen (or, more generally, of any one-electron atom) in the Lyman series.It is emitted when the atomic electron transitions from an n = 2 orbital to the ground state (n = 1), where n is the principal quantum number.

  4. Hydrogen spectral series - Wikipedia

    en.wikipedia.org/wiki/Hydrogen_spectral_series

    The spectral lines are grouped into series according to n′. Lines are named sequentially starting from the longest wavelength/lowest frequency of the series, using Greek letters within each series. For example, the 2 → 1 line is called "Lyman-alpha" (Ly-α), while the 7 → 3 line is called "Paschen-delta" (Pa-δ).

  5. Hydrogen-alpha - Wikipedia

    en.wikipedia.org/wiki/Hydrogen-alpha

    For the Lyman series the naming convention is: n = 2 to n = 1 is called Lyman-alpha, n = 3 to n = 1 is called Lyman-beta, etc. H-alpha has a wavelength of 656.281 nm, [1] is visible in the red part of the electromagnetic spectrum, and is the easiest way for astronomers to trace the ionized hydrogen content of gas clouds.

  6. Lyman continuum photons - Wikipedia

    en.wikipedia.org/wiki/Lyman_continuum_photons

    Lyman-alpha blob; Lyman-alpha forest; Lyman-break galaxy; Lyman series; Haro 11 - One of the two galaxies in the local universe that 'leaks' Lyman continuum photons. Tololo-1247-232 - The second galaxy in the local universe that 'leaks' Lyman continuum photons. Pea galaxy - Many nearby Green Peas are confirmed LyC 'leakers'. [5] [6] Reionization

  7. Reionization - Wikipedia

    en.wikipedia.org/wiki/Reionization

    The Lyman alpha line is the n=2 to n=1 transition of neutral hydrogen, and can be produced copiously by galaxies with young stars. [11] Moreover, Lyman alpha photons interact strongly with neutral hydrogen in intergalactic gas through resonant scattering, wherein neutral atoms in the ground (n=1) state absorb Lyman alpha photons and almost ...

  8. Here’s why voters were notified of Richard Lyman’s withdrawal ...

    www.aol.com/why-voters-were-notified-richard...

    On Oct. 26, Phil Lyman’s campaign issued a press release that acknowledged the withdrawal of Richard Lyman from the race and also referenced allegations of Richard Lyman being paid to run by Gov ...

  9. Lyman-alpha emitter - Wikipedia

    en.wikipedia.org/wiki/Lyman-alpha_emitter

    The Lyman-alpha line in most LAEs is thought to be caused by recombination of interstellar hydrogen that is ionized by an ongoing burst of star formation. Such Lyman alpha emission was first suggested as a signature of young galaxies by Bruce Partridge and P. J. E. Peebles in 1967. [ 1 ]