Radio detection of nebulae around four luminous blue variable stars in the Large Magellanic Cloud

The nebulae associated with four luminous blue variables (LBVs) in the Large Magellanic Cloud (LMC) have been observed at 5.5 and 9GHz using the Australia Telescope Compact Array, and radio emission has been detected for first time in sources R127, R143, S61 and S119. The radio maps of the nebulae h...

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Main Authors: Agliozzo, C., Umana, G., Trigilio, C., Buemi, C., Leto, P., Ingallinera, A., Franzen, Thomas, Noriega-Crespo, A.
Format: Journal Article
Published: Oxford University Press 2012
Online Access:http://hdl.handle.net/20.500.11937/52857
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author Agliozzo, C.
Umana, G.
Trigilio, C.
Buemi, C.
Leto, P.
Ingallinera, A.
Franzen, Thomas
Noriega-Crespo, A.
author_facet Agliozzo, C.
Umana, G.
Trigilio, C.
Buemi, C.
Leto, P.
Ingallinera, A.
Franzen, Thomas
Noriega-Crespo, A.
author_sort Agliozzo, C.
building Curtin Institutional Repository
collection Online Access
description The nebulae associated with four luminous blue variables (LBVs) in the Large Magellanic Cloud (LMC) have been observed at 5.5 and 9GHz using the Australia Telescope Compact Array, and radio emission has been detected for first time in sources R127, R143, S61 and S119. The radio maps of the nebulae have an angular resolution of ~1.5arcsec and a sensitivity of 1.5-3.0 × 10 -2mJybeam -1 and show a very similar morphology to that observed in Ha. This similarity permits us to assume that the Ha emission is not affected by strong intrinsic extinction due to dust within the nebulae. We estimate the masses of ionized gas in the LBV nebulae and find values consistent with those measured in Galactic LBVs. © 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS.
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institution Curtin University Malaysia
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publishDate 2012
publisher Oxford University Press
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spelling curtin-20.500.11937-528572017-09-13T21:24:57Z Radio detection of nebulae around four luminous blue variable stars in the Large Magellanic Cloud Agliozzo, C. Umana, G. Trigilio, C. Buemi, C. Leto, P. Ingallinera, A. Franzen, Thomas Noriega-Crespo, A. The nebulae associated with four luminous blue variables (LBVs) in the Large Magellanic Cloud (LMC) have been observed at 5.5 and 9GHz using the Australia Telescope Compact Array, and radio emission has been detected for first time in sources R127, R143, S61 and S119. The radio maps of the nebulae have an angular resolution of ~1.5arcsec and a sensitivity of 1.5-3.0 × 10 -2mJybeam -1 and show a very similar morphology to that observed in Ha. This similarity permits us to assume that the Ha emission is not affected by strong intrinsic extinction due to dust within the nebulae. We estimate the masses of ionized gas in the LBV nebulae and find values consistent with those measured in Galactic LBVs. © 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS. 2012 Journal Article http://hdl.handle.net/20.500.11937/52857 10.1111/j.1365-2966.2012.21791.x Oxford University Press fulltext
spellingShingle Agliozzo, C.
Umana, G.
Trigilio, C.
Buemi, C.
Leto, P.
Ingallinera, A.
Franzen, Thomas
Noriega-Crespo, A.
Radio detection of nebulae around four luminous blue variable stars in the Large Magellanic Cloud
title Radio detection of nebulae around four luminous blue variable stars in the Large Magellanic Cloud
title_full Radio detection of nebulae around four luminous blue variable stars in the Large Magellanic Cloud
title_fullStr Radio detection of nebulae around four luminous blue variable stars in the Large Magellanic Cloud
title_full_unstemmed Radio detection of nebulae around four luminous blue variable stars in the Large Magellanic Cloud
title_short Radio detection of nebulae around four luminous blue variable stars in the Large Magellanic Cloud
title_sort radio detection of nebulae around four luminous blue variable stars in the large magellanic cloud
url http://hdl.handle.net/20.500.11937/52857