Discovery of spectacular quasar-driven superbubbles in red quasars
Quasar-driven outflows on galactic scales are a routinely invoked ingredient for galaxy formation models. We report the discovery of ionized gas nebulae surrounding three luminous red quasars at z ~ 0.4 from Gemini integral field unit observations. All these nebulae feature unprecedented pairs of “s...
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| Hauptverfasser: | , , , , , , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
Jul 2023
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| In: |
Science advances
Year: 2023, Jahrgang: 9, Heft: 28, Pages: 1-13 |
| ISSN: | 2375-2548 |
| DOI: | 10.1126/sciadv.adg8287 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: https://doi.org/10.1126/sciadv.adg8287 Verlag, kostenfrei, Volltext: https://www.science.org/doi/10.1126/sciadv.adg8287 |
| Verfasserangaben: | Lu Shen, Guilin Liu, Zhicheng He, Nadia L. Zakamska, Eilat Glikman, Jenny E. Greene, Weida Hu, Guobin Mou, Dominika Wylezalek, David S.N. Rupke |
| Zusammenfassung: | Quasar-driven outflows on galactic scales are a routinely invoked ingredient for galaxy formation models. We report the discovery of ionized gas nebulae surrounding three luminous red quasars at z ~ 0.4 from Gemini integral field unit observations. All these nebulae feature unprecedented pairs of “superbubbles” extending ~20 kpc in diameter, and the line-of-sight velocity difference between the red- and blueshifted bubbles reaches up to ~1200 km/s. Their spectacular dual-bubble morphology (in analogy to the galactic “Fermi bubbles”) and their kinematics provide unambiguous evidence for galaxy-wide quasar-driven outflows, in parallel with the quasi-spherical outflows similar in size from luminous type 1 and type 2 quasars at concordant redshift. These bubble pairs manifest themselves as a signpost of the short-lived superbubble “break-out” phase, when the quasar wind drives the bubbles to escape the confinement from the dense environment and plunge into the galactic halo with a high-velocity expansion. |
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| Beschreibung: | Online veröffentlicht: 12. Juli 2023 Gesehen am 09.10.2023 |
| Beschreibung: | Online Resource |
| ISSN: | 2375-2548 |
| DOI: | 10.1126/sciadv.adg8287 |