The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission in Active Galactic Nuclei - IOPscience
6. Stellar spectra
Balmer Series - an overview | ScienceDirect Topics
White-light flare emission
Amazon | High-Resolution Continuum Source AAS: The Better Way to Do Atomic Absorption Spectrometry | Welz, Bernhard, Becker-Ross, Helmut, Florek, Stefan, Heitmann, Uwe | Analytic
3.10 Hydrogen Spectral Series
Eight per cent leakage of Lyman continuum photons from a compact, star-forming dwarf galaxy | Nature
The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission in Active Galactic Nuclei - IOPscience
Fritz11
Electron Transitions and Formation of the Spectra (Chapter 2) - Spectroscopy for Amateur Astronomers
Profiles of the Balmer β (2–4), Balmer η (2–9), and Paschen η (3–10)... | Download Scientific Diagram
Tracing the origins of permitted emission lines in RU Lupi down to AU scales
AGN Emission Lines - H. Netzer
PDF) Zeeman- and Paschen-Back-effect of the hyperfine structure of the sodiumD 1-line | Maurizio E Musso - Academia.edu
Paschen and Balmer hydrogen lines correlation in Be stars - Scientific Amateur Astronomy - Cloudy Nights
Electron Transitions and Formation of the Spectra (Chapter 2) - Spectroscopy for Amateur Astronomers
Flux-calibrated continuum-subtracted Paschen β for all 13 epochs. The... | Download Scientific Diagram
The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission in Active Galactic Nuclei - IOPscience
Paschen and Balmer hydrogen lines correlation in Be stars - Scientific Amateur Astronomy - Cloudy Nights
The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission in Active Galactic Nuclei - IOPscience
1: Paschen curve of ammonia [Rad68]. The vertical lines indicate the pd... | Download Scientific Diagram
Modelling of the Paschen series of HR 1861 with our non-LTE (ADS)... | Download Scientific Diagram
In the given figure, the energy levels of hydrogen atom have been shown along with some transitions marked A, B, C, D and E.The transitions A, B and C respectively represent :
RVS spectrum of the Be star HIP 55044. Both the Ca ii and the Paschen... | Download Scientific Diagram
Left: Map of T e derived from the magnitude of the Paschen continuum... | Download Scientific Diagram
Themes > Science > Astronomy > Modern Astronomy > The Interaction of Light and Matter > Atomic Absorption and Emission Spectra