AustralieFrV1, Main, Exploration, bibRecord, 007200

Radio observations of NGC 6388: an upper limit on the mass of its central black hole

Identifieur interne : 007200 ( Main/Exploration ); précédent : 007199; suivant : 007201

Radio observations of NGC 6388: an upper limit on the mass of its central black hole

Auteurs : D. Cseh [France] ; P. Kaaret [États-Unis] ; S. Corbel [France] ; E. Körding [France] ; M. Coriat [France] ; A. Tzioumis [Australie] ; B. Lanzoni [Italie]

Source :

Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2010-08-01.

RBID : ISTEX:3D9B41FBFDF251514AA0CFB33DF60EBB21CD1DDE

Descripteurs français

Pascal (Inist)
- Amas globulaire, Amas stellaire, Borne supérieure, Continuum, Cosmologie, Disque accrétion, Gravité, Incertitude, Luminosité, Observation radio, Trou noir.
Wicri :
- topic : Cosmologie, Niveau sonore.

English descriptors

Abstract

We present the results of deep radio observations with the Australia Telescope Compact Array (ATCA) of the globular cluster NGC 6388. We show that there is no radio source detected (with an rms noise level of 27 μJy) at the cluster centre of gravity or at the locations of any of the Chandra X‐ray sources in the cluster. Based on the fundamental plane of accreting black holes which is a relationship between X‐ray luminosity, radio luminosity and black hole mass, we place an upper limit of ∼1500 M on the mass of the putative intermediate‐mass black hole located at the centre of NGC 6388. We discuss the uncertainties of this upper limit and the previously suggested black hole mass of based on surface density profile analysis.

Url:

DOI: 10.1111/j.1365-2966.2010.16726.x

Affiliations:

Le document en format XML

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<term>Black hole mass</term>
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<front><div type="abstract" xml:lang="en">We present the results of deep radio observations with the Australia Telescope Compact Array (ATCA) of the globular cluster NGC 6388. We show that there is no radio source detected (with an rms noise level of 27 μJy) at the cluster centre of gravity or at the locations of any of the Chandra X‐ray sources in the cluster. Based on the fundamental plane of accreting black holes which is a relationship between X‐ray luminosity, radio luminosity and black hole mass, we place an upper limit of ∼1500 M on the mass of the putative intermediate‐mass black hole located at the centre of NGC 6388. We discuss the uncertainties of this upper limit and the previously suggested black hole mass of based on surface density profile analysis.</div>
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Radio observations of NGC 6388: an upper limit on the mass of its central black hole

Radio observations of NGC 6388: an upper limit on the mass of its central black hole

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Descripteurs français

English descriptors

Abstract

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