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6. Stellar spectra
6. Stellar spectra

The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission  in Active Galactic Nuclei - IOPscience
The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission in Active Galactic Nuclei - IOPscience

6. Stellar spectra
6. Stellar spectra

Balmer Series - an overview | ScienceDirect Topics
Balmer Series - an overview | ScienceDirect Topics

White-light flare emission
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
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
3.10 Hydrogen Spectral Series

Eight per cent leakage of Lyman continuum photons from a compact,  star-forming dwarf galaxy | Nature
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
The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission in Active Galactic Nuclei - IOPscience

Fritz11
Fritz11

Electron Transitions and Formation of the Spectra (Chapter 2) -  Spectroscopy for Amateur Astronomers
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
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
Tracing the origins of permitted emission lines in RU Lupi down to AU scales

AGN Emission Lines - H. Netzer
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
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
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
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
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
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
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
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
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
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 :
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
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
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
Themes > Science > Astronomy > Modern Astronomy > The Interaction of Light and Matter > Atomic Absorption and Emission Spectra