Two-phase character of the interstellar medium in nebulae around quasars

Details Two-phase character of the interstellar medium in nebulae around quasars Two-phase character of the interstellar medium in nebulae around quasars

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..499z&link_type=abstract

Astrofizika (ISSN 0571-7132), vol. 27, Dec. 1987, p. 499-507. In Russian.

Astronomy and Astrophysics

Astronomy

Gas Temperature, Interstellar Gas, Molecular Clouds, Nebulae, Quasars, Rarefied Gases, Gas Density, High Temperature Gases

Scientific paper

A theoretical analysis shows that interstellar gas in nebulae around
quasars is thermally unstable and that it breaks down into two phases:
cold (T = 10,000 K) dense clouds and hot (100-million K) rarefied media.
The density, radius, and mass of the clouds formed as a result of the
thermal instability are evaluated.

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