SMC HI shells velocities : J/MNRAS/289/225


Authors : Staveley-Smith L. orcid , Sault R.J., Hatzidimitriou D. (hide) , Sault R.J., Hatzidimitriou D. et..al

Bibcode : 1997MNRAS.289..225S (ADS) (Simbad) (Objects) (hide)

CDS Keywords : Magellanic Clouds; H I data; Radial velocities
UAT : Magellanic Clouds, H I line emission, Radial velocity

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Inserted into VizieR : 23-Feb-1998
Last modification : 25-Jun-2024

An H I aperture synthesis mosaic of the Small Magellanic Cloud (1997)

Keywords : surveys - ISM atoms - ISM: kinematics and dynamics - galaxies: kinematics and dynamics - Magellanic Clouds - radio lines: ISM

Abstract:We present the results of a survey of neutral hydrogen emission in the Small Magellanic Cloud (SMC) with the Australia Telescope Compact Array (ATCA). The survey consists of a mosaic of 320 separate pointings of the 375-m array, resulting in a resolution of 1.6arcmin (28pc, for a distance of 60kpc) over a field of 20deg^2^. The rms brightness temperature sensitivity is 1.4K, corresponding to an H I column density sensitivity of 4x^18^cm^-2^ for each velocity channel of width 1.6km/s. The HI distribution is complex and, on scales <=1kpc, appears to be dominated by the effects of expanding H I shells, which are probably driven by the combined effects of supernovae and stellar winds from massive stars. The picture of the ...(more)
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Lister Staveley-Smith

                
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