4,186 research outputs found
Jet-dominated quiescent state in black hole X-ray binaries: the cases of A0620--00 and XTE J1118+480
The radiative mechanism of the black hole X-ray transients (BHXTs) in their
quiescent states (defined as the 2-10 keV X-ray luminosity ) remains unclear. In this work, we investigate the
quasi-simultaneous quiescent state spectrum (including radio, infrared,
optical, ultraviolet and X-ray) of two BHXTs, A0620--00 and XTE J1118+480. We
find that, these two sources can be well described by a coupled accretion --
jet model. More specifically, most of the emission (radio up-to infrared, and
the X-ray waveband) comes from the collimated relativistic jet. Emission from
hot accretion flow is totally insignificant, and it can only be observed in
mid-infrared (the synchrotron peak). Emission from the outer cold disc is only
evident in UV band. These results are consistent with our previous
investigation on the quiescent state of V404 Cyg, and confirm that the
quiescent state is jet-dominated.Comment: 11 pages, 1 figure, accepted for publication in Research in Astronomy
and Astrophysic
BCR algorithm and the theorem
We show using the Beylkin-Coifman-Rokhlin algorithm in the Haar basis that
any singular integral operator can be written as the sum of a bounded operator
on , , and of a perfect dyadic singular integral operator.
This allows to deduce a local theorem for singular integral operators
from the one for perfect dyadic singular integral operators obtained by
Hofmann, Muscalu, Thiele, Tao and the first author.Comment: Change of title. New abstract and new introductio
Jet-dominated quiescent states in black hole X-ray binaries: the case of V404 Cyg
The dynamical and radiative properties of the quiescent state (X-ray
luminosity ) of black hole X-ray transients
(BHXTs) remains unclear, mainly because of low-luminosity and poor data
quantity. We demonstrate that, the simultaneous multi-wavelength (including
radio, optical, ultraviolet and X-ray bands) spectrum of V404 Cyg in its bright
quiescent state can be well described by the radiation from the companion star
and more importantly, the compact jet. Neither the outer thin disc nor the
inner hot accretion flow is important in the total spectrum. Together with
several additional recent findings, i.e. the power-law X-ray spectrum and the
constant X-ray spectral shape (or constant photon index) in contrast to the
dramatic change in the X-ray luminosity, we argue the quiescent state spectrum
of BHXTs is actually jet-dominated. Observational features consistent with this
jet model are also discussed as supporting evidences.Comment: accepted for the publication in MNRAS Letters, 5 pages, 2 figure
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