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...

Bibliografiset tiedot
Päätekijät:	Thomas A. Gomez, Mark C. Zammit, Igor Bray, Christopher J. Fontes, Jackson R. White, Harold Johnson
Aineistotyyppi:	Artikkeli
Kieli:	English
Julkaistu:	IOP Publishing 2024-01-01
Sarja:	The Astrophysical Journal
Aiheet:	Atomic spectroscopy Atomic physics Neutron stars Stellar atmospheres
Linkit:	https://doi.org/10.3847/1538-4357/ad8f34

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