X-ray absorption effects due to intergalactic abundance of carbon

Details X-ray absorption effects due to intergalactic abundance of carbon X-ray absorption effects due to intergalactic abundance of carbon

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..67..201r&link_type=abstract

Astrophysics and Space Science, vol. 67, no. 1, Jan. 1980, p. 201-204.

Astronomy and Astrophysics

Astrophysics

2

Abundance, Carbon, Intergalactic Media, X Ray Absorption, Astronomical Models, Density (Mass/Volume), Extragalactic Radio Sources, Red Shift

Scientific paper

The absorption effects at soft X-ray and hard ultraviolet wavelengths due to a model abundance of intergalactic carbon material have been investigated for different cosmologies. Even though the local density, 1.0 x 10 to the -34th g/cu cm, of the absorbing component of the intergalactic material in the form of carbon is not adequate for the thermalization of the discrete background radiation, the amount of absorption in X-rays up to the Hubble radius is not negligible.

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