YOUNG STARLESS CORES EMBEDDED IN THE MAGNETICALLY DOMINATED PIPE NEBULA. II. EXTENDED DATASET
收藏arXiv2012-07-14 更新2024-08-06 收录
下载链接：
http://arxiv.org/abs/1207.3310v1
下载链接
链接失效反馈官方服务：
资源简介：
本数据集包含对Pipe星云中九个年轻无星核的观测，重点关注其物理和化学特性。通过使用IRAM 30米望远镜，对1.2毫米尘埃连续辐射进行映射，并对分子线进行观测。这些核位于星云的不同区域，具有不同的密度和化学成分，为研究恒星形成早期的条件提供了良好的实验室。数据集包括尘埃连续辐射图和分子线观测，以及相关的物理和化学参数，如密度、质量和化学丰度，有助于理解这些核的演化和恒星形成过程。
This dataset contains observations of nine young starless cores in the Pipe Nebula, with a focus on their physical and chemical properties. Using the IRAM 30m Telescope, we mapped the 1.2 mm dust continuum emission and conducted observations of molecular lines. These cores are located in different regions of the nebula, with varying densities and chemical compositions, providing an excellent laboratory for studying the conditions during the early stages of star formation. The dataset includes dust continuum maps, molecular line observations, and relevant physical and chemical parameters such as density, mass, and chemical abundances, which aid in understanding the evolution of these cores and the star formation process.
提供机构：
Institut de Ci`encies de l’Espai (CSIC-IEEC), Campus UAB, Facultat de Ci`encies, Torre C-5p, 08193 Bellaterra, Catalunya, Spain
创建时间：
2012-07-14
