'Hidden masses' and the dynamic evolution of stellar systems

Details 'Hidden masses' and the dynamic evolution of stellar systems 'Hidden masses' and the dynamic evolution of stellar systems

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977afz....13..271a&link_type=abstract

Astrofizika, vol. 13, May 1977, p. 271-274. In Russian.

Astronomy and Astrophysics

Astrophysics

Galactic Structure, Star Distribution, Stellar Evolution, Stellar Mass, Stellar Systems, Astronomical Models, Astrophysics, Dynamic Models

Scientific paper

The dynamic evolution of stellar systems containing 'hidden masses' is analyzed. The results show that the compact objects which can account for 'hidden masses', such as faint low-mass stars and cold blobs of neutral hydrogen, are probably a peculiar population that could not have originated in common with the normal visible population of galaxies. It is suggested that if 'hidden-mass' compact objects are detected by direct observations, they might constitute a Population III in stellar systems.

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