Deep Hα survey of the Milky Way - IV. The l = 301o to l = 324o area
Deep Hα survey of the Milky Way - IV. The l = 301o to l = 324o area
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银河系深 Hα 巡天 - IV. l = 301o 至 l = 324o 区域
DOI：
10.1051/aas:1998406
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发表时间：
1998
期刊：
影响因子：
--
通讯作者：
M. Marcelin
中科院分区：
文献类型：
--
作者：
D. Russeil;Y. Georgelin;P. Amram;J. Gach;Y. Georgelin;M. Marcelin
离子化氢的详细速度场在l = 301和l = 324之间被观测到，作为对南银河系H α巡天的一部分。对H α剖面的分析显示了6种不同的速度分量。这些H α观测，结合多波长和恒星数据，被用来找出不同气体层的最可能距离。
The detailed velocity field of the ionized hydrogen has been observed between l = 301 0 and l = 324 0 as part of an H α Survey of the southern Milky Way. Analysis of the H α profiles shows six different velocity components. These H α observations, combined with multiwavelength and stellar data, are used to find the most probable distances of the different gas layers.