银河系存在翘曲的证据

Back to the Galaxy Pub Date : 2008-05-29 DOI:10.1063/1.43975
H. Freudenreich, T. J. Sodroski, G. Berriman, E. Dwek, B. Franz, M. Hauser, T. Kelsall, S. Moseley, N. Odegard, R. Silverberg, G. Toller, J. Weiland
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引用次数: 0

摘要

在宇宙背景探测器漫射红外背景实验(DIRBE)的数据中发现了银河系盘表面亮度分布的大规模扭曲。在远红外波段,它在尘埃的热发射中可见。在近红外波段,它在星光中可见。远红外翘曲与速度积分HI相匹配。近红外翘曲方向大致相同,但振幅较小,随波长增加而增大。这与银河系的恒星盘以与HI层相同的方式弯曲一致。
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Dirbe evidence for a warp in the Galaxy
A large‐scale warp in the surface brightness distribution of the Galactic disk has been found in the data of the Diffuse Infrared Background Experiment (DIRBE) of the Cosmic Background Explorer. In the far‐infrared it is seen in seen in thermal emission by dust. In the near‐infrared it is seen in starlight. The far‐infrared warp matches that of the velocity‐integrated HI. The near‐infrared warp has approximately the same orientation, but has a smaller amplitude, which increases with increasing wavelength. This is consistent with the stellar disk of the Galaxy being bent in the same way as the HI layer.
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