Spectra Used In New Temperature and Turbulent Velocity Measurements of the LISM
收藏DataCite Commons2022-07-01 更新2025-04-09 收录
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http://archive.stsci.edu/doi/resolve/resolve.html?doi=10.17909/gabn-m136
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资源简介：
Analysis of interstellar absorption lines observed in high-resolution HST spectra of nearby stars provides temperatures, turbulent velocities, and kinetic properties of warm interstellar clouds. A new analysis reveals a wide range of temperatures and turbulent velocities within the Local Interstellar Cloud (LIC) and the nearby Cluster of Interstellar Clouds (CLIC). New measurements of temperature and turbulent velocity are made from fits to HI, DI, CII, OI, MgI, MgII, and FeII and listed in Tables 2 and 3 in Linsky, Redfield, Ryder, & Chasan-Taber (2022).
提供机构：
STScI/MAST
创建时间：
2022-07-01
