Published online by Cambridge University Press: 12 April 2016
High-dispersion Copernicus and IUE observations of chromospheric Ly α emission are used to study the distribution of HI in the local interstellar medium. Interstellar parameters are derived toward 3 stars within 5 pc of the sun, and upper limits are given for the Ly a flux from 9 other stars within 10 pc.
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