Synchrotron emission from radio to X-rays in the Low/Hard spectral state

By Sera M arko, H. Falcke, Robert P. Fender. 2001

197 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/77700df63872de6ccb98f4415e851991b23eeade

Citations in the corpus

• The structure of the nuclear stellar cluster of the Milky Way (2006, unknown): “Also, there a theoretical and observational arguments that favour the presence of a jet in Sgr A* (e.g., Melia & Falcke 2001; Markoff et al. 2001; Yuan et al. 2002; Bower et al. 2004).”
• Hard X‐ray states and radio emission in GRS 1915+105 (2001, unknown): “During the hard state (C) the X-ray spectrum is dominated by a power law component, which is widely accepted to originate from inverse Compton processes in the inner geometrically thick accretion flow (such as a corona and/or an ADAF), although there are alternatives (e.g. Markoff et al. 2001).”
• The Stellar Cusp around the Supermassive Black Hole in the Galactic Center (2003, unknown): “…rate also agrees with recent theoretical models of the Sgr A* spectral energy distribution, including its X-ray emission (Liu & Melia 2002; Markoff et al. 2001) but is 2–3 orders of magnitude lower than earlier models based on advectiondominated accretion flows (ADAFs; Narayan et al.…”
• Hot Accretion Flows Around Black Holes (2014, unknown): “4.1.4 Alternative models of Sgr A* Two alternative models of Sgr A* have been discussed in the literature: the jet model (Falcke & Markoff 2000, Markoff et al. 2001, Yuan et al. 2002a, Markoff et al. 2007), and the spherical accretion model (Melia 1992, Melia et al. 2001).”
• First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon (2021, unknown): “We use a specific, but widely explored (e.g., Özel et al. 2000; Markoff et al. 2001; Yuan et al. 2003), description for electron acceleration, namely that accelerated electrons add a power-law tail to the thermal distribution function.”
• Global optical/infrared-X-ray correlations in X-ray binaries: quantifying disc and jet contributions (2006, unknown): “4jet (Blandford & Konigl 1979; Falcke & Biermann 1996; Markoff et al. 2001).”
• Modelling the behaviour of accretion flows in X-ray binaries (2007, unknown): “Models where the X-rays are produced directly in the jet were proposed by Markoff et al. (2001).”
• A Long, Hard Look at the Low/Hard State in Accreting Black Holes (2006, unknown): “Markoff et al. (2001) suggested that all of the hard X-ray emission in XTE J1118+480 may be due to the steady, compact jet implied by radio observations.”
• A radio-emitting outflow in the quiescent state of A0620−00: implications for modelling low-luminosity black hole binaries (2006, unknown): “It has been suggested that the outflow, and not the inflow of gas, could be responsible for the hard X-ray power law which dominates the spectrum of hard state BHBs (Falcke & Bierman 1995; Markoff et al. 2001; Giannios 2005).”
• Correlations between X-ray and radio spectral properties of accreting black holes (2002, unknown): “This power-law spectral variability when extended to the turnover energy (when the synchrotron source becomes optically thick) at ∼1 eV (e.g. Markoff et al. 2001, 2003) would imply variability below this energy by a factor of ∼102.”
• A Jet-ADAF model for Sgr A* (2001, unknown): “In that case, a corresponding optically thin power-law spectrum at IR/optical frequencies is generally expected, as is seen in many AGN and perhaps even X-ray binary jets (e.g., Markoff et al. 2001a).”