Constraining jet physics in weakly accreting black holes
Abstract
Outflowing jets are observed in a variety of astronomical objects such as accreting compact objects from X-ray binaries (XRBs) to active galactic nuclei (AGN), as well as at stellar birth and death. Yet we still do not know exactly what they are comprised of, why and how they form, or their exact relationship with the accretion flow. In this talk I focus on jets in black hole systems, which provide the ideal test population for studying the relationship between inflow and outflow over an extreme range in mass and accretion rate.
- Publication:
-
Black Holes from Stars to Galaxies -- Across the Range of Masses
- Pub Date:
- April 2007
- DOI:
- 10.1017/S1743921307004863
- Bibcode:
- 2007IAUS..238..145M
- Keywords:
-
- Black hole physics accretion;
- accretion disks;
- radiation mechanisms: nonthermal;
- X-rays: binaries;
- galaxies: active;
- galaxies: jets