Revisiting FUSE O vi Emission in Galaxy Halos
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ac04af/pdf
Reference36 articles.
1. UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10
2. The galactic fountain of high-velocity clouds
3. EMPIRICALLY CONSTRAINED PREDICTIONS FOR METAL-LINE EMISSION FROM THE CIRCUMGALACTIC MEDIUM
4. Detection of the Diffuse H i Emission in the Circumgalactic Medium of NGC 891 and NGC 4565
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1. UV Cooling via O VI Emission in the Superwind of M82 Observed with the Far Ultraviolet Spectroscopic Explorer (FUSE);The Astronomical Journal;2024-06-11
2. Disc-halo gas outflows driven by stellar clusters as seen in multiwavelength tracers;Monthly Notices of the Royal Astronomical Society;2023-01-27
3. Absorption-based circumgalactic medium line emission estimates;Monthly Notices of the Royal Astronomical Society;2022-08-25
4. Aspera: the UV SmallSat telescope to detect and map the warm-hot gas phase in nearby galaxy halos;UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts X;2021-08-20
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