A morphological search for molecular shells and cavities was performed around 63 Galactic supernova remnants (SNRs) at 10 ≤ l ≤ 50, ∣b∣ ≤ 1 using the FOREST Unbiased Galactic Imaging survey with the Nobeyama 45 m telescope CO-line data at high-angular (20″) and high-velocity (1.3 km s⁻¹) resolutions. The results are presented as supplementary data for general purpose investigations of the interaction between SNRs and interstellar matter in the form of an atlas of CO-line maps superposed on radio continuum maps at 20 cm along with a list of their kinematic distances determined from CO-line radial velocities.

中文翻译：

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带有FUGIN的银河系超新星遗迹周围的CO线壳和腔图集FUGIN：森林（我们的45 m望远镜的光束接收器系统）用Nobeyama 45 m望远镜进行无偏银河平面成像调查。

用于分子壳和空腔的形态学搜索在10≤执行约为63银河超新星遗迹（信噪比）升|≤50，b在高≤1使用与野边山45米望远镜CO线数据森林无偏银河成像调查|角度（20英寸）和高速（1.3 km s ^-1）分辨率。结果以补充数据的形式提供，用于常规研究SNR和星际物质之间的相互作用，形式为CO线图集的地图集，该图集叠加在20 cm的无线电连续性图上，并列出了从CO-线径向速度。