Detecting galactic hydrogen line emission

Details Detecting galactic hydrogen line emission Detecting galactic hydrogen line emission

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phyed..30....9h&link_type=abstract

Physics Education, Volume 30, Issue 1, pp. 9-14 (1995).

Physics

Physics Education

Scientific paper

Hydrogen gas clouds dispersed throughout our own galaxy, the Milky Way, emit radio waves at a frequency of 1420 MHz. This article details a system incorporating mainly amateur radio communication equipment to observe and profile these galactic hydrogen radio emissions. Subsequent analysis of hydrogen line profiles can reveal the spiral structure of our galaxy.

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