Radio and UV observations of high latitude HI

Details Radio and UV observations of high latitude HI Radio and UV observations of high latitude HI

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2345..290l&link_type=abstract

In NASA. Goddard Space Flight Center Local Interstellar Medium, No. 81 p 290 (SEE N85-15539 06-90)

Astronomy and Astrophysics

Astronomy

Hydrogen, Lyman Alpha Radiation, Neutral Gases, Stars, Radio Astronomy, Sun, Ultraviolet Astronomy

Scientific paper

Interstellar Lyman alpha observations toward high latitude stars, which give the column density of H I between Earth and the star, and 21 cm radio observations, which give the total H I column density to and beyond the star, can be combined to map out the amount of neutral gas as a function of distance from the Sun. Observations of the 21 cm and Lyman alpha lines made toward approximately 50 high latitude OB stars are presented. These data are used to discuss the distribution of H I in the solar neighborhood.

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