Modeling Competing Line-broadening Mechanisms in Neutron Star Atmospheres: Interference between Motional Stark and Ion Broadening

Modeling Competing Line-broadening Mechanisms in Neutron Star Atmospheres: Interference between Motional Stark and Ion Broadening

Neutron star surfaces have extremely high magnetic fields. In the atmosphere, the broadening of spectral lines will be substantial from the dense plasma as well as from the magnetic field. One broadening mechanism of note is due to the motional Stark effect (MSE)—an additional electric field that ar...

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Bibliografische gegevens
Hoofdauteurs: Thomas A. Gomez, Mark C. Zammit, Igor Bray, Christopher J. Fontes, Jackson R. White, Harold Johnson
Formaat: Artikel
Taal:English
Gepubliceerd in: IOP Publishing 2024-01-01
Reeks:The Astrophysical Journal
Onderwerpen:
Atomic spectroscopy
Atomic physics
Neutron stars
Stellar atmospheres
Online toegang:https://doi.org/10.3847/1538-4357/ad8f34

Internet

https://doi.org/10.3847/1538-4357/ad8f34

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