The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O vii, O viii, and Fe L-shell Transitions

The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O vii, O viii, and Fe L-shell Transitions

The XMM-Newton Line Emission Analysis Program (X-LEAP) is designed to study diffuse X-ray emissions from the Milky Way (MW) hot gas, as well as emissions from the foreground solar wind charge exchange (SWCX). This paper presents an all-sky survey of spectral feature intensities corresponding to the...

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Bibliographic Details
Main Authors: Zeyang Pan, Zhijie Qu, Joel N. Bregman, Jifeng Liu
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Supplement Series
Subjects:
the Milky Way
Diffuse x-ray background
Circumgalactic medium
Solar wind
Online Access:https://doi.org/10.3847/1538-4365/ad2ea0

Internet

https://doi.org/10.3847/1538-4365/ad2ea0

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