Bright phase in galactic evolution and ionization of intergalactic gas

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

7

Galactic Evolution, Gas Ionization, Intergalactic Media, Red Shift, Gas Temperature, Ionizing Radiation, Optical Thickness, Thermal Radiation, Thomson Scattering

Scientific paper

Conditions are investigated under which ionization of intergalactic gas is possible at large redshifts as a result of thermal radiation from young galaxies passing through the bright phase of their evolution. Parameters of the ionizing radiation are evaluated for different models of galactic chemical evolution, and it is shown that total ionization may occur if the redshift corresponding to the beginning of the bright phase does not exceed certain values. The intergalactic-gas temperature in the ionization zone is obtained analytically along with the maximum redshift allowing total ionization. The maximum optical depth of the intergalactic gas to Thompson scattering is determined as a function of the luminosity of young galaxies as well as the moment of initiation and the duration of the bright phase. It is concluded that the optical depths required by the vortex theory of galaxy formation in order to explain the small-scale isotropy of relict radiation do not fall outside the limits of either the maximum optical depth or the applicability of the theory itself.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Bright phase in galactic evolution and ionization of intergalactic gas 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 Bright phase in galactic evolution and ionization of intergalactic gas, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bright phase in galactic evolution and ionization of intergalactic gas will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1781949

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.