X-Ray halos

Details X-Ray halos X-Ray halos

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975xrat.rept..193s&link_type=abstract

In ESA X-Ray Astronomy and Related Topics p 193-202 (SEE N76-11958 02-89)

Astronomy and Astrophysics

Astronomy

Esa Satellites, Halos, Interstellar Matter, Satellite Observation, X Ray Sources, Cosmic Dust, Grain Boundaries, Lunar Occultation, Point Sources, Scattering Cross Sections, Size Determination, X Ray Scattering

Scientific paper

The possibilities of observing interstellar grain from halo formations onboard the EXOSAT satellite are considered. The characteristics of halos and grain properties are outlined. It is shown that halo observations can be performed with the EXOSAT medium energy instrument in the occultation mode, and with the low energy instrument in both the occultation and arbitrary pointing mode.

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