We use Chandra, HST and VLA observations of M87 to investigate the physics of X-ray emission from AGN jets. We find that X-ray hotspots in the M87 jet occur primarily in regions with hard optical-to-X-ray spectra and lower than average polarization. Particle injection appears to be required both continuously in the jet sheath as well as locally at X-ray hotspots
The Chandra X-ray Observatory has proven to be a vital tool for studying high-energy emission proces...
There is good evidence for X-ray emission associated with AGN jets which are relativistically booste...
We present the evidence for X-ray variability from the core and from knot A in the M87 jet based on ...
M87 hosts a 3–6 billion solar mass black hole with a remarkable relativistic jet that has been regul...
We present the first high resolution X-ray image of the jet in M 87 using the Chandra X-ray Observat...
The supermassive black hole, M87, has long been a target of interest for the study of black hole phy...
We study the contribution of thermal and non-thermal processes to the inverse Compton emission of th...
The Chandra X-ray Observatory has proven to be a vital tool for studying high-energy emission proces...
The jet in 3C273 is a high-power quasar jet with radio, optical and X-ray emission whose size and br...
Approximately 10% of active galactic nuclei exhibit relativistic jets, which are powered by the accr...
We present the results from an X-ray and optical survey of a sample of 17 radio jets in AGN performe...
A significant fraction of known galaxies contain an active galactic nucleus (AGN) at their cores, th...
A new interpretation of the optical knot in the jet of M87, HST-1, is presented. High sensitivity 22...
Horizon-scale observations of the jetted active galactic nucleus M87 are compared with simulations s...
The X-ray emission from the jets in active galactic nuclei (AGN) carries important information on th...
The Chandra X-ray Observatory has proven to be a vital tool for studying high-energy emission proces...
There is good evidence for X-ray emission associated with AGN jets which are relativistically booste...
We present the evidence for X-ray variability from the core and from knot A in the M87 jet based on ...
M87 hosts a 3–6 billion solar mass black hole with a remarkable relativistic jet that has been regul...
We present the first high resolution X-ray image of the jet in M 87 using the Chandra X-ray Observat...
The supermassive black hole, M87, has long been a target of interest for the study of black hole phy...
We study the contribution of thermal and non-thermal processes to the inverse Compton emission of th...
The Chandra X-ray Observatory has proven to be a vital tool for studying high-energy emission proces...
The jet in 3C273 is a high-power quasar jet with radio, optical and X-ray emission whose size and br...
Approximately 10% of active galactic nuclei exhibit relativistic jets, which are powered by the accr...
We present the results from an X-ray and optical survey of a sample of 17 radio jets in AGN performe...
A significant fraction of known galaxies contain an active galactic nucleus (AGN) at their cores, th...
A new interpretation of the optical knot in the jet of M87, HST-1, is presented. High sensitivity 22...
Horizon-scale observations of the jetted active galactic nucleus M87 are compared with simulations s...
The X-ray emission from the jets in active galactic nuclei (AGN) carries important information on th...
The Chandra X-ray Observatory has proven to be a vital tool for studying high-energy emission proces...
There is good evidence for X-ray emission associated with AGN jets which are relativistically booste...
We present the evidence for X-ray variability from the core and from knot A in the M87 jet based on ...