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 |
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