Numerical Models for Sgr A*

Details Numerical Models for Sgr A* Numerical Models for Sgr A*

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21321002g&link_type=abstract

American Astronomical Society, AAS Meeting #213, #210.02; Bulletin of the American Astronomical Society, Vol. 41, p.282

Astronomy and Astrophysics

Astronomy

Scientific paper

Using numerical simulations it is possible to evolve a nearly ab initio model for a magnetized accretion flow near a rotating black hole, and to calculate the emergent radiation if cooling is weak. I will describe how such models might constrain the spin, accretion rate and inclination of an accretion flow in Sgr A*. I will also catalog the strengths, weaknesses, and future prospects of the models.

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