The Large-scale Ionization Cones in the Galaxy

There is compelling evidence for a highly energetic Seyfert explosion (1056-57 erg) that occurred in the Galactic center a few million years ago. The clearest indications are the X-ray/γ-ray "10 kpc bubbles" identified by the ROSAT and Fermi satellites. In an earlier paper, we suggested an...

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Veröffentlicht in:	The Astrophysical journal 2019-11, Vol.886 (1), p.45
Hauptverfasser:	Bland-Hawthorn, Joss, Maloney, Philip R., Sutherland, Ralph, Groves, Brent, Guglielmo, Magda, Li, Wenhao, Curzons, Andrew, Cecil, Gerald, Fox, Andrew J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Bubbles Clouds Cones Corona Emission Galaxies galaxies: active galaxies: Seyfert Galaxy: evolution Galaxy: nucleus H alpha line Hubble Space Telescope Ionization Ionizing radiation Luminosity Radiation radiation mechanisms: non-thermal Satellites Seyfert galaxies shock waves Space telescopes Stars & galaxies Stellar coronas Stellar models Stellar populations Stellar winds Time dependence Ultraviolet absorption Wind Wind models
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