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ID: 5558.0, MPI für Astrophysik / Cosmology
Redshifts of new galaxies
Authors:Arp, H.
Language:English
Publisher:ASTRONOMICAL SOC PACIFIC
Place of Publication:SAN FRANCISCO
Date of Publication (YYYY-MM-DD):1999
Start Page:347
End Page:355
Title of Series:IAU SYMPOSIA
Review Status:Peer-review
Audience:Not Specified
Abstract / Description:Observations increasingly demonstrate the spatial association of high redshift objects with larger, low redshift galaxies. These companion objects show a continuous range of physical properties - from very compact, high redshift quasars, through smaller active galaxies and finally to only slightly smaller companion galaxies of slightly higher redshift. The shift in energy distribution from high to low makes it clear that are seeing an empirical evolution from newly created to older, more normal galaxies. In order to account for the evolution of intrinsic redshift we must conclude that matter is initially born with low mass particles whose mass increase with time (age). This requires a physics which is nonlocal (Machian) and which is therefore more applicable to the cosmos than the Big Bang extrapolation of local physics. Ambartsumian's "superfluid" foresaw some of the properties of the new, low particle mass, protogalactic plasma which is required, demonstrating again the age-old lesson that open minded observation is much more powerful than theoretical assumptions. Since the ejected plasma, which preferentially emerges along the minor axis of the parent galaxy, develops into an entire galaxy, accretion disks cannot supply sufficient material. New matter must be created within a "white hold" rather than bouncing old matter off a "black hole".
External Publication Status:published
Document Type:Conference-Paper
Communicated by:N. N.
Affiliations:MPI für Astrophysik
External Affiliations:Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85740; Garching, Germany; Max Planck Inst Astrophys, D-85740 Garching, Germany
Identifiers:ISI:000175726500063
ISSN:0074-1809
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