X ray absorption by dark nebulae (HEAO-2 guest investigator program)

Details X ray absorption by dark nebulae (HEAO-2 guest investigator program) X ray absorption by dark nebulae (HEAO-2 guest investigator program)

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991wisc.reptq....s&link_type=abstract

Final Report Wisconsin Univ., Madison. Dept. of Physics.

Physics

Dark Matter, Diffuse Radiation, Emission Spectra, Nebulae, X Ray Absorption, X Ray Sources, Background Radiation, C Band, Galactic Radiation, Heao 2, Imaging Techniques, Interstellar Chemistry, Proportional Counters

Scientific paper

A study is described of data obtained from the Imaging Proportional Counter (IPC) x ray detector aboard the HEAO-2 satellite (Einstein Observatory). The research project involved a search for absorption of diffuse low energy x ray background emission by galactic dark nebulae. The commonly accepted picture that the bulk of the C band emission originates locally, closer that a few hundred parsec, and the bulk of the M band emission originates farther away than a few hundred parsec, was tested. The idea was to look for evidence of absorption of the diffuse background radiation by nearby interstellar clouds.

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