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The velocity structure of the local interstellar medium probed by ultra high resolution spectroscopy

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Figure

Table 1. List of the nearby stars observed for the interstellar Ca K line using the UHRF
Fig. 1. The interstellar Ca K lines observed with the UHRF. The observed data are plotted as histograms
Table 2. Line profile parameters for the interstellar Ca K lines shown in Fig. 1, compared with other published values; a colon indicates thata previously published value is uncertain
Fig. 2. a An expanded view of the central narrow (− 21. 3 km s−1)component towards 51 Oph, showing the asymmetry of the line pro-file

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