Maps of the spatially resolved line-of-sight velocity field of the Milky Way Interstellar Medium made with Kinetic Tomography

Maps of the line-of-sight velocity field of the Milky Way ISM as a function of position in the Galactic plane. All velocities are in the heliocentric frame. The procedure for deriving the gas and dust KT map is described in Kinetic Tomography. I. A Method for Mapping the Milky Way’s Interstellar Medium in Four Dimensions. (https://doi.org/10.3847/1538-3881/153/1/8). The procedure for deriving the DIB KT map is described in Kinetic Tomography. II. A second method for mapping the velocity field of the Milky Way Interstellar Medium and a comparison with spiral structure models. This paper is currently under review. A pre-print is available on arXiv: https://arxiv.org/abs/1808.01286.

本数据集包含银河系星际介质（Interstellar Medium, ISM）的视线速度场随银道面位置变化的分布图。
所有速度均采用日心系参考框架。
气体与尘埃动力学层析成像（Kinetic Tomography, KT）图的推导流程详见论文《Kinetic Tomography. I. A Method for Mapping the Milky Way’s Interstellar Medium in Four Dimensions》，其DOI链接为：https://doi.org/10.3847/1538-3881/153/1/8。
弥散星际带（Diffuse Interstellar Bands, DIB）动力学层析成像图的推导流程详见论文《Kinetic Tomography. II. A second method for mapping the velocity field of the Milky Way Interstellar Medium and a comparison with spiral structure models》，该论文目前处于同行评审阶段，预印本可于arXiv平台获取：https://arxiv.org/abs/1808.01286。