中文

高氘丰度分子云核:Nobeyama巡天测绘

星系天体物理 2022-05-26 v1

摘要

我们展示了使用Nobeyama 45米望远镜在82-94 GHz分子N2_2H+^+、HC3_3N和CCS发射线对包含107个SCUBA-2核的44个视场进行的on-the-fly测绘观测结果。本研究旨在调查具有高氘丰度且可能接近恒星形成起始的核的物理性质。我们发现N2_2H+^+和HC3_3N线发射的分布近似类似于850-μ\mum尘埃连续发射的分布,而CCS线发射通常未被探测到或分布为环绕850-μ\mum尘埃连续发射峰值位置的团块状结构。偶尔(12%),我们观测到作为年轻恒星天体早期气体示踪物的CCS发射,可能由于局部高激发。向恒星形成的演化不会立即影响非热速度弥散。

关键词

引用

@article{arxiv.2106.04052,
  title  = {Molecular Cloud Cores with High Deuterium Fractions: Nobeyama Mapping Survey},
  author = {Ken'ichi Tatematsu and Gwanjeong Kim and Tie Liu and Neal J. Evans and Hee-Weon Yi and Jeong-Eun Lee and Yuefang Wu and Naomi Hirano and Sheng-Yuan Liu and Somnath Dutta and Dipen Sahu and Patricio Sanhueza and Kee-Tae Kim and Mika Juvela and L. Viktor T'oth and Orsolya Feh'er and Jinhua He and J. X. Ge and Siyi Feng and Minho Choi and Miju Kang and Mark A. Thompson and Gary A. Fuller and Di Li and Isabelle Ristorcelli and Ke Wang and James Di Francesco and David Eden and Satoshi Ohashi and Ryo Kandori and Charlotte Vastel and Tomoya Hirota and Takeshi Sakai and Xing Lu and Quang Nguyen Lu'o'ng and Hiroko Shinnaga and Jungha Kim and JCMT Large Program "SCOPE'' collaboration},
  journal= {arXiv preprint arXiv:2106.04052},
  year   = {2022}
}

备注

45 pages, 15 figures, ApJS, in press