Mass pick-up in astronomical flows

Details Mass pick-up in astronomical flows Mass pick-up in astronomical flows

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.144..615h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 144, no. 1-2, May 1988, p. 615-627.

Astronomy and Astrophysics

Astrophysics

52

Quasars, Solar Wind, Star Formation, Stellar Mass Accretion, Stellar Winds, Supernova Remnants, Mass Flow, Solar System, Stellar Coronas, Wolf-Rayet Stars

Scientific paper

Many astrophysical sources are clumpy. The flows in the diffuse media in these sources are affected by the mass picked up through the ablation of the embedded clumps. The diffuse media-clump interfaces can be observable sources themselves. Flows in clumpy stellar wind blown bubbles, supernova remnants, quasar winds, cooling gas accretion on to galaxies, and in pre-galactic bubbles blown by energy input from young galaxies, are discussed. Pick-up has important chemical as well as dynamical effects in star forming regions. The natures of the interfaces are considered.

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