Finite-lens Effect on Self-lensing in Detached White Dwarfs-main Sequence Binary Systems

In edge-on and detached binary systems, including a white dwarf (WD) and a main-sequence (MS) star system (or WDMS), when the source star is passing behind the compact companion its light is bent and magnified. Meanwhile, some part of its image’s area is obscured by the WD’s disk. These two effects...

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Hlavní autoři:	Sedighe Sajadian, Hossein Fatheddin
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2024-01-01
Edice:	The Astronomical Journal
Témata:	Astronomical simulations Eclipsing binary stars Compact binary stars Gravitational lensing Occultation White dwarf stars
On-line přístup:	https://doi.org/10.3847/1538-3881/ad81d1
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