The unification of relativistic jets
arXiv:1310.5822 · doi:10.1142/S2010194514601884
Abstract
I report about the unification of relativistic jets from compact objects. The mass range is between 1.4 and 10 billion solar masses (i.e. from neutron stars to supermassive black holes in galaxies).
6 pages, 1 figure. Proceedings HEPROIV (Heidelberg, Germany, 23-26 July 2013). Some typo fixed. To be published on International Journal of Modern Physics Conference Series
References in corpus (5)
- A Universal Scaling for the Energetics of Relativistic Jets From Black Hole Systems
- Refining the fundamental plane of accreting black holes
- Jet-dominated advective systems: radio and X-ray luminosity dependence on the accretion rate
- Powerful relativistic jets in narrow-line Seyfert 1 galaxies
- Where to look for radiatively inefficient accretion flows (and find them)
Cited by in corpus (21)
- Properties of flat-spectrum radio-loud Narrow-Line Seyfert 1 Galaxies
- Radio-emitting narrow-line Seyfert 1 galaxies in the JVLA perspective
- Radio jet emission from GeV-emitting narrow-line Seyfert 1 galaxies
- Absorbed relativistic jets in radio-quiet narrow-line Seyfert 1 galaxies
- The relativistic jet and its central engine of blazars
- Kiloparsec-scale emission in the narrow-line Seyfert 1 galaxy Mrk 783
- The obstructed jet in Mrk 231
- Radio morphology of southern narrow-line Seyfert 1 galaxies with Very Large Array observations
- Broadband X-ray observations of four gamma-ray narrow-line Seyfert 1 galaxies
- Line shapes in narrow-line Seyfert 1 galaxies: a tracer of physical properties?
- Properties of the narrow line Seyfert 1 galaxies revisited
- Interactions between the jet and disk wind in a nearby radio intermediate quasar III Zw 2
- Modelling the variable emission states of -ray emitting Narrow-Line Seyfert 1 galaxies
- Quantitative comparisons of VHE gamma-ray blazar flares with relativistic reconnection models
- The radio structure of the -ray narrow-line Seyfert 1 galaxy SDSS J211852.96073227.5
- Long-term Swift and Metsähovi monitoring of SDSS J164100.10+345452.7 reveals multi-wavelength correlated variability
- The host galaxy of low-luminosity compact sources
- An optical perspective on early-stage AGN with extreme radio flares
- Investigating the origin of radio emission in candidate super-Eddington accreting black holes
- Intra-night optical variability study of a non-jetted narrow-line Seyfert 1 galaxy: SDSS J163401.94+480940.1
- Calibrating the power of relativistic jets