甘油：用于高质量星形成区域的诊断工具
天体物理学
2017-01-18 v1
摘要
我们在此提出一种创新的技术，用于处理从观测到的甘油多线光谱中推导物理参数的难题，方法是基于大速度梯度近似计算的合成光谱对所有线的同时拟合；通过数值方法找到最佳物理参数。
引用
@article{arxiv.astro-ph/0402014,
title = {Methanol: a diagnostic tool for high-mass star-forming regions},
author = {S. Leurini and P. Schilke and K. M. Menten and D. R. Flower and J. T. Pottage and L. -H Xu},
journal= {arXiv preprint arXiv:astro-ph/0402014},
year = {2017}
}
备注
4 pages, 2 figures. (Co)authored by members of the MPIfR (Sub)millimeter Astronomy Group. To appear in the Proceedings of the 4th Cologne-Bonn-Zermatt-Symposium "The Dense Interstellar Medium in Galaxies" eds. S. Pfalzner, C. Kramer, C. Straubmeier, & A. Heithausen (Springer: Berlin)