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首页> 外文会议>International Meeting on High Energy Gamma-Ray Astronomy >Non-thermal radiation from molecular clouds illuminated by cosmic rays from nearby supernova remnants.
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Non-thermal radiation from molecular clouds illuminated by cosmic rays from nearby supernova remnants.

机译：来自附近的超新星残余的宇宙射线照射的分子云的非热辐射。

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Molecular clouds are expected to emit non-thermal radiation due to cosmic ray interactions in the dense magnetizedgas. Such emission is amplified if a cloud is located close to an accelerator of cosmic rays and if cosmic rays can leave theaccelerator and diffusively reach the cloud. We consider the situation in which a molecular cloud is located in the proximity ofa supernova remnant which is accelerating cosmic rays and gradually releasing them into the interstellar medium. We calculatethe multiwavelength spectrum from radio to γ-rays which emerges from the cloud as the result of cosmic ray interactions. Thetotal energy output is dominated by the γ-ray emission, which can exceed the emission from other bands by an order ofmagnitude or more. This suggests that some of the unidentified TeV sources detected so far, with no obvious or very weakcounterpart in other wavelengths, might be associated with clouds illuminated by cosmic rays coming from a nearby source.
机译：预期分子云引起的致密磁化节中的宇宙射线相互作用引起的非热辐射。如果云位于靠近宇宙射线的加速器，并且宇宙射线可以离开灰色的速度并扩散到达云，则这种发射被放大。我们认为分子云位于邻近的超新加达残余物的情况下，其加速宇宙射线并逐渐将它们释放到星际介质中。根据宇宙射线相互作用，我们将来自无线电与γ射线的多波长光谱计算出来，从云中出现。随着γ射线发射的γ射线输出是由γ射线发射的主导，这可以通过造成的顺序超过其他频带的排放。这表明到目前为止检测到的一些未识别的TEV来源，在其他波长中没有明显或非常弱，可能与来自附近来源的宇宙光线照射的云相关联。

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