Background cosmological radiation

Details Background cosmological radiation Background cosmological radiation

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987esasp.268...57l&link_type=abstract

In ESA Space Astronomy and Solar System Exploration p 57-62 (SEE N87-29374 23-88)

Astronomy and Astrophysics

Astronomy

Background Radiation, Big Bang Cosmology, Cosmic Noise, Relic Radiation, Anisotropic Media, Cosmic Gases, Cosmic X Rays, Intergalactic Media, Microwaves

Scientific paper

At any wavelength of the electromagnetic spectrum, the sky is not dark between the stars (or other objects). A diffuse component - a background - is present, very difficult to detect for various reasons: its low level, the parasit contributions of different phenomena and the difficulty of absolute calibrations of the detectors. In this introductive talk, the author will concentrate of the two spectral domains of greatest cosmological interest: the millimetric, with the Cosmic Microwave Background and the X-ray, with the possible emission from intergalactic gas.

Affiliated with

Also associated with

No associations

Rating

Background cosmological radiation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Background cosmological radiation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Background cosmological radiation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-857959