Clark, James; Steele, I. A. and Fender, R. P.
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|DOI (Digital Object Identifier) Link:||http://doi.org/10.1046/j.1365-8711.1998.01848.x|
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We present the first radio observations of a sample of 13 optically and IR bright southern hemisphere classical Be stars made from the Australian Telescope Compact Array at 3.5cm and 6.3cm simultaneously. One star, Cen was detected at 3.5cm and a second, ? Cen was also thought to have been detected; further observations of this source are required to confirm this detection. No sources were detected at 6.3cm, although Cen was previously detected at this wavelength by other observers at a higher flux than our detection limit. The radio observations show that the spectral energy distribution undergoes a turnover between the far IR and radio wavelengths, as was seen in previous studies. Likewise we find no simple correlation between far IR and radio flux. Lower limits to the outer disc radius were found to be of the order of few hundred solar radii; of the order of those found previously by Taylor et al.
|Item Type:||Journal Article|
|Keywords:||Be stars; Stars; Circumstellar matter; Radio stars; Emission-line stars|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Users 9108 not found.|
|Date Deposited:||28 Jul 2009 14:41|
|Last Modified:||02 Aug 2016 14:55|
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