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...

Bibliográfalaš dieđut
Váldodahkkit:	Thomas A. Gomez, Mark C. Zammit, Igor Bray, Christopher J. Fontes, Jackson R. White, Harold Johnson
Materiálatiipa:	Artihkal
Giella:	English
Almmustuhtton:	IOP Publishing 2024-01-01
Ráidu:	The Astrophysical Journal
Fáttát:	Atomic spectroscopy Atomic physics Neutron stars Stellar atmospheres
Liŋkkat:	https://doi.org/10.3847/1538-4357/ad8f34

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