首页> 外文期刊>PASJ: Publications of the Astronomical Society of Japan >Catalogue of ~(12)CO(J = 1-0) and ~(13)CO(J = 1-0) Molecular Cloudsin the Carina Flare Supershell
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Catalogue of ~(12)CO(J = 1-0) and ~(13)CO(J = 1-0) Molecular Cloudsin the Carina Flare Supershell

机译:船Fla火炬超壳中〜(12)CO(J = 1-0)和〜(13)CO(J = 1-0)分子云的目录

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摘要

We present a catalogue of ~(12)CO(J = 1-0) and ~(13)molecular clouds in the spatio-velocity rangeof the Carina Flare supershell, GSH 287+04-17. The data cover a region of 66 square degrees and were takenwith the NANTEN 4 m telescope, at spatial and velocity resolutions of 2:6 and 0.1 km s-I . Decomposition of theemission results in the identification of 156 ~(12)CO clouds and 60 ~(13)clouds, for which we provide observational andphysical parameters. Previous work suggests the majority of the detected mass forms part of a comoving molecularcloud complex that is physically associated with the expanding shell. The cloud internal velocity dispersions, degreeof virialization and size-linewidth relations are found to be consistent with those of other Galactic samples. However,the vertical distribution is heavily skewed towards high-altitudes. The robust association of high-z molecular cloudswith a known supershell provides some observational backing for the theory that expanding shells contribute to thesupport of a high-altitude molecular layer.
机译:我们提出了在Cari​​na Flare超壳GSH 287 + 04-17的时速范围内的〜(12)CO(J = 1-0)和〜(13)分子云的目录。数据覆盖66平方度的区域,是使用NANTEN 4 m望远镜拍摄的,空间和速度分辨率分别为2:6和0.1 km s-I。发射的分解可识别156〜(12)CO云和60〜(13)云,为此我们提供了观测和物理参数。先前的工作表明,大部分检测到的质量形成了与不断膨胀的壳物理相关的共同移动的分子云复合体的一部分。发现云的内部速度散布,玻璃化程度和大小线宽关系与其他银河系样本的一致。但是,垂直分布严重偏向高海拔。高z分子云与已知的超壳之间的牢固联系为扩展壳有助于高海拔分子层的支撑的理论提供了一些观察依据。

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