QUIJOTE scientific results – VI. The Haze as seen by QUIJOTE

ABSTRACT The Haze is an excess of microwave intensity emission surrounding the Galactic Centre. It is spatially correlated with the γ-ray Fermi bubbles, and with the S-PASS radio polarization plumes, suggesting a possible common provenance. The models proposed to explain the origin of the Haze, incl...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2023-01, Vol.519 (3), p.3460-3480
Hauptverfasser: Guidi, F, Génova-Santos, R T, Rubiño-Martín, J A, Peel, M W, Fernández-Torreiro, M, López-Caraballo, C H, Vignaga, R, de la Hoz, E, Vielva, P, Watson, R A, Ashdown, M, Dickinson, C, Artal, E, Barreiro, R B, Casas, F J, Herranz, D, Hoyland, R J, Lasenby, A N, Martinez-Gonzalez, E, Piccirillo, L, Poidevin, F, Rebolo, R, Ruiz-Granados, B, Tramonte, D, Vansyngel, F
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Sprache:eng
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