Michael Yeung
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    • The SRG/eROSITA diffuse soft X-ray background II. spectra and morphology of the eROSITA bubbles in the western Galactic hemisphere
    • Determination of the Solar System contribution to the soft x-ray sky
    • Low-mass stars dominate the hot (0.7 keV) Galactic X-ray emission
    • Study and reproducibility of the SRG/eROSITA background with particle rejection on and off
    • The SRG/eROSITA all-sky survey: View of the Fornax galaxy cluster
    • The SRG/eROSITA All-Sky Survey: Large-scale view of the Centaurus cluster
    • The hot circumgalactic medium in the eROSITA All-Sky Survey: III. Star-forming and quiescent galaxies
    • The Distance to Dobashi 6193—A Dark Cloud Shadowing the eROSITA Bubbles
    • The Distance to Dobashi 6193—A Dark Cloud Shadowing the eROSITA Bubbles
    • The SRG/eROSITA diffuse soft X-ray background: I. The local hot bubble in the western Galactic hemisphere
    • The SRG/eROSITA diffuse soft X-ray background: I. The local hot bubble in the western Galactic hemisphere
    • The SRG/eROSITA All-Sky Survey: Large-scale view of the Centaurus cluster
    • SRG/eROSITA X-ray shadowing study of giant molecular clouds
    • SRG/eROSITA X-ray shadowing study of giant molecular clouds
    • Recent Formation of a Spiral Disk Hosting Progenitor Globular Clusters at the Center of the Perseus Brightest Cluster Galaxy. I. Spiral Disk
    • Recent Formation of a Spiral Disk Hosting Progenitor Globular Clusters at the Center of the Perseus Brightest Cluster Galaxy. I. Spiral Disk
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Recent Formation of a Spiral Disk Hosting Progenitor Globular Clusters at the Center of the Perseus Brightest Cluster Galaxy. I. Spiral Disk

Mar 1, 2022·
Michael C. H. Yeung
,
Youichi Ohyama
,
Jeremy Lim
· 0 min read
Cite DOI arXiv NASA ADS
Type
Journal Article
Publication
ApJ
Last updated on Mar 1, 2022
Astrophysics - Astrophysics of Galaxies
← Recent Formation of a Spiral Disk Hosting Progenitor Globular Clusters at the Center of the Perseus Brightest Cluster Galaxy. I. Spiral Disk Mar 1, 2022

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