Atomic and molecular data for observations of the interstellar medium with the hubble space telescope
作者： Donald C. Morton
DOI: 10.1007/BFB0040312
关键词: Pillars of Creation 、 Hubble Deep Field South 、 Astrophysics 、 Interstellar medium 、 Physics 、 Astronomy 、 Line (formation) 、 Hubble Deep Field 、 Digicon 、 Hubble Ultra-Deep Field 、 Spectrograph
摘要: The high resolution spectrograph on HST, with resolving powers up to 94000 or 3.2 km s−1, is giving us a new look at interstellar absorption lines in the range 1090 3350 A. signal-to-noise ratios possible digicon detectors provide precise line profiles suitable for studying individual velocity components.
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