One-temperature accretion flows with advection and nonthermal e+/- pair production

Details One-temperature accretion flows with advection and nonthermal e+/- pair production One-temperature accretion flows with advection and nonthermal e+/- pair production

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cha%26a..22..386y&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 22, Issue 4, p. 386-394.

Astronomy and Astrophysics

Astrophysics

Scientific paper

By means of the self-similar relations of the hot flow with advection and nonthermal e+/- pair production, we examine the radial structure of such a flow. Some typical features have been confirmed, and several new results obtained: there exists a critical radius rcr; the local cooling rate is inversely proportional to the square of the mass of the central object; the pair density in the accretion flow with advection is higher than in the SLE disk.

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