A jet model for the broadband spectrum of XTE J1118+480: Synchrotron emission from radio to X-rays in the Low/Hard spectral state
Sera Markoff (MPIfR Bonn), Heino Falcke (MPIfR Bonn), Rob Fender, (Univ. Amsterdam)

TL;DR
This paper presents a jet model that explains the broadband spectrum of XTE J1118+480, from radio to X-rays, primarily through synchrotron emission from a relativistic jet, challenging traditional accretion models.
Contribution
It introduces a simple jet-based model that accounts for the entire broadband spectrum of XTE J1118+480, emphasizing synchrotron emission as the dominant process in the Low/Hard state.
Findings
Broadband spectrum fit by synchrotron emission from jet
X-ray emission explained as synchrotron from shock regions
Spectral cutoff determined by plasma parameters
Abstract
Observations have revealed strong evidence for powerful jets in the Low/Hard states of black hole candidate X-ray binaries. Correlations, both temporal and spectral, between the radio -- infrared and X-ray bands suggest that jet synchrotron as well as inverse Compton emission could also be significantly contributing at higher frequencies. We show here that, for reasonable assumptions about the jet physical parameters, the broadband spectrum from radio through X-rays can be almost entirely fit by synchrotron emission. We explore a relatively simple model for a relativistic, adiabatically expanding jet combined with a truncated thermal disk conjoined by an ADAF, in the context of the recently discovered black hole binary XTE J1118+480. In particular, the X-ray power-law emission can be explained as optically thin synchrotron emission from a shock acceleration region in the innermost part…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astrophysics and Cosmic Phenomena · Pulsars and Gravitational Waves Research
