Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.177..391d&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 177, Nov. 1976, p. 391-408.
Astronomy and Astrophysics
Astrophysics
7
Astronomical Models, Gravitational Collapse, Quasars, Red Shift, Star Clusters, Astrophysics, Distribution Functions, Hydrodynamic Equations, Life (Durability), Velocity Distribution
Scientific paper
Physical properties of a class of static spherically symmetric collapsed objects capable of giving high internal gravitational redshifts have been studied in order to investigate their plausibility as models for high-redshift quasi-stellar objects (QSOs). Calculations have been made for these models to investigate their binding energy and their stability against small radial oscillations. Calculations of the velocity distribution function are made to study the extent to which such models can be looked upon as star cluster. Thermal and hydrodynamic time scales of such models are calculated. Assuming the star cluster scenario, the geometrical obscuration of the light emitted by the central region is estimated.
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