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The physical parameters of the microquasar S26 in the Sculptor Group galaxy NGC 7793

Date

Authors

Dopita, Michael

Payne, J L

Filipovic, M D

Pannuti, Thomas G

Publisher

Blackwell Publishing Ltd

Abstract

NGC 7793-S26 is an extended source (350pc × 185pc) previously studied in the radio, optical and X-ray domains. It has been identified as a microquasar which has inflated a superbubble. We used integral-field spectra from the Wide-Field Spectrograph on th

Keywords

Keywords: Galaxies: individual: NGC 7793; ISM: abundances; ISM: bubbles; ISM: jets and outflows; Stars: winds, outflows; X-rays: binaries

URI

http://hdl.handle.net/1885/69360

Collections

ANU Research Publications

Source

Monthly Notices of the Royal Astronomical Society

Type

Journal article

Access Statement

Open Access

DOI

10.1111/j.1365-2966.2012.21947.x

Downloads

File

Description

01_Dopita_The_physical_parameters_of_the_2012.pdf (664.61 KB)