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Planck view of the M?82 galaxy

机译:M?82星系的普朗克视图

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Planck data towards the galaxy M?82 are analyzed in the 70, 100 and 143 GHz bands. A substantial north-south and east-west temperature asymmetry is found, extending up to 1° from the galactic center. Being almost frequency-independent, these temperature asymmetries are indicative of a Doppler-induced effect regarding the line-of-sight dynamics on the halo scale, the ejections from the galactic center and, possibly, even the tidal interaction with M?81 galaxy. The temperature asymmetry thus acts as a model-independent tool to reveal the bulk dynamics in nearby edge-on spiral galaxies, like the Sunyaev-Zeldovich effect for clusters of galaxies.
机译:在70、100和143 GHz频段分析了朝向M?82星系的普朗克数据。发现了南北和东西向的温度不对称现象,从银河系中心一直延伸到1°。这些温度不对称性几乎与频率无关,表示在晕圈尺度上的视线动力学,从银河系中心的射出,甚至可能与M?81星系的潮汐相互作用有关的多普勒效应。因此,温度不对称性是一种独立于模型的工具,用于揭示附近边缘螺旋星系的整体动力学,例如星系团的Sunyaev-Zeldovich效应。

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