Galaxy formation after Z = 1000

Details Galaxy formation after Z = 1000 Galaxy formation after Z = 1000

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980rspta.296..289j&link_type=abstract

(Royal Society, Discussion on the Origin and Early Evolution of the Galaxies, London, England, Feb. 14, 15, 1979.) Royal Society

Astronomy and Astrophysics

Astronomy

4

Astronomical Models, Galactic Evolution, Gravitational Effects, Red Shift, Background Radiation, Gravitational Collapse, Hierarchies, Microwaves

Scientific paper

The 'hierarchical clustering' and 'pancake' theories for galaxy formation are reviewed. In spite of the considerable difference between these two schemes it is difficult to offer observational tests that might discriminate whether galaxies or clusters of galaxies formed first. Recent observations of the microwave background radiation spectrum suggest that one may be looking back to the time of galaxy formation, and future isotropy measurements below 1 mm may provide vital clues.

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