AustralieFrV1, Main, Exploration, bibRecord, 007249

Limits on the quiescent radio emission from the black hole binaries GRO J1655−40 and XTE J1550−564

Identifieur interne : 007249 ( Main/Exploration ); précédent : 007248; suivant : 007250

Limits on the quiescent radio emission from the black hole binaries GRO J1655−40 and XTE J1550−564

Auteurs : D. E. Calvelo [Royaume-Uni] ; R. P. Fender ; D. M. Russell [Pays-Bas] ; E. Gallo [États-Unis] ; S. Corbel [France] ; A. K. Tzioumis [Australie] ; M. E. Bell ; F. Lewis ; T. J. Maccarone

Source :

Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2010-12-01.

RBID : ISTEX:AC1BBB9F3BB59FBFEC70D233115CA255D30A9371

Descripteurs français

Pascal (Inist)
- Binaire RX, Binaire serrée, Borne supérieure, Corrélation, Cosmologie, Densité flux, Emission radioélectrique, Flux radioélectrique, Jet, Luminosité, Observation RX, Observation optique, Observation radio, Quiescence, Rayon X dur, Source RX binaire, Source RX cosmique, Trou noir.
Wicri :
- topic : Cosmologie.

English descriptors

Abstract

We present the results of radio observations of the black hole binaries GRO J1655−40 and XTE J1550−564 in quiescence, with the upgraded Australia Telescope Compact Array. Neither system was detected. Radio flux density upper limits (3σ) of 26 μJy (at 5.5 GHz), 47 μJy (at 9 GHz) for GRO J1655−40 and 1.4 mJy (at 1.75 GHz), 27 μJy (at 5.5 GHz), 47 μJy (at 9 GHz) for XTE J1550−564 were measured. In conjunction with quasi‐simultaneous Chandra X‐ray observations (in the case of GRO J1655−40) and Faulkes Telescope optical observations (XTE J1550−564) we find that these systems provide the first evidence of relatively ‘radio‐quiet’ black hole binaries at low luminosities, indicating that the scatter observed in the hard state X‐ray–radio correlation at higher luminosities may also extend towards quiescent levels.

Url:

DOI: 10.1111/j.1365-2966.2010.17348.x

Affiliations:

Le document en format XML

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<front><div type="abstract" xml:lang="en">We present the results of radio observations of the black hole binaries GRO J1655−40 and XTE J1550−564 in quiescence, with the upgraded Australia Telescope Compact Array. Neither system was detected. Radio flux density upper limits (3σ) of 26 μJy (at 5.5 GHz), 47 μJy (at 9 GHz) for GRO J1655−40 and 1.4 mJy (at 1.75 GHz), 27 μJy (at 5.5 GHz), 47 μJy (at 9 GHz) for XTE J1550−564 were measured. In conjunction with quasi‐simultaneous Chandra X‐ray observations (in the case of GRO J1655−40) and Faulkes Telescope optical observations (XTE J1550−564) we find that these systems provide the first evidence of relatively ‘radio‐quiet’ black hole binaries at low luminosities, indicating that the scatter observed in the hard state X‐ray–radio correlation at higher luminosities may also extend towards quiescent levels.</div>
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Limits on the quiescent radio emission from the black hole binaries GRO J1655−40 and XTE J1550−564

Limits on the quiescent radio emission from the black hole binaries GRO J1655−40 and XTE J1550−564

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Descripteurs français

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Abstract

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