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- Publisher Website: 10.1111/j.1365-2966.2006.10279.x
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Article: Radio observations of the planetary nebula around the OHIR star OH 354.88-0.54 (V1018 Sco)
Title | Radio observations of the planetary nebula around the OHIR star OH 354.88-0.54 (V1018 Sco) |
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Authors | |
Keywords | Stars: AGB and post-AGB Masers Radiation mechanisms: non-thermal Planetary nebulae: general |
Issue Date | 2006 |
Citation | Monthly Notices of the Royal Astronomical Society, 2006, v. 369, n. 1, p. 189-196 How to Cite? |
Abstract | We present radio observations of the unique, recently formed, planetary nebula (PN) associated with a very long-period OHIR variable star V1018 Sco that is unequivocally still in its asymptotic giant branch phase. Two regions within the optical nebula are clearly detected in non-thermal radio continuum emission, with radio spectral indices comparable to those seen in colliding-wind Wolf-Rayet binaries. We suggest that these represent shocked interactions between the hot, fast stellar wind and the cold nebular shell that represents the PN's slow wind moving away from the central star. This same interface produces both synchrotron radio continuum and the optical PN emission. The fast wind is neither spherical in geometry nor aligned with any obvious optical or radio axis. We also report the detection of transient H 2O maser emission in this nebula. © 2006 RAS. |
Persistent Identifier | http://hdl.handle.net/10722/208851 |
ISSN | 2023 Impact Factor: 4.7 2023 SCImago Journal Rankings: 1.621 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Cohen, Martin G. | - |
dc.contributor.author | Chapman, Jessica M. | - |
dc.contributor.author | Deacon, Rachel M. | - |
dc.contributor.author | Sault, Robert J. | - |
dc.contributor.author | Parker, Quentin A. | - |
dc.contributor.author | Green, Anne J. | - |
dc.date.accessioned | 2015-03-23T02:01:56Z | - |
dc.date.available | 2015-03-23T02:01:56Z | - |
dc.date.issued | 2006 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, 2006, v. 369, n. 1, p. 189-196 | - |
dc.identifier.issn | 0035-8711 | - |
dc.identifier.uri | http://hdl.handle.net/10722/208851 | - |
dc.description.abstract | We present radio observations of the unique, recently formed, planetary nebula (PN) associated with a very long-period OHIR variable star V1018 Sco that is unequivocally still in its asymptotic giant branch phase. Two regions within the optical nebula are clearly detected in non-thermal radio continuum emission, with radio spectral indices comparable to those seen in colliding-wind Wolf-Rayet binaries. We suggest that these represent shocked interactions between the hot, fast stellar wind and the cold nebular shell that represents the PN's slow wind moving away from the central star. This same interface produces both synchrotron radio continuum and the optical PN emission. The fast wind is neither spherical in geometry nor aligned with any obvious optical or radio axis. We also report the detection of transient H 2O maser emission in this nebula. © 2006 RAS. | - |
dc.language | eng | - |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | - |
dc.subject | Stars: AGB and post-AGB | - |
dc.subject | Masers | - |
dc.subject | Radiation mechanisms: non-thermal | - |
dc.subject | Planetary nebulae: general | - |
dc.title | Radio observations of the planetary nebula around the OHIR star OH 354.88-0.54 (V1018 Sco) | - |
dc.type | Article | - |
dc.description.nature | link_to_OA_fulltext | - |
dc.identifier.doi | 10.1111/j.1365-2966.2006.10279.x | - |
dc.identifier.scopus | eid_2-s2.0-33745235062 | - |
dc.identifier.volume | 369 | - |
dc.identifier.issue | 1 | - |
dc.identifier.spage | 189 | - |
dc.identifier.epage | 196 | - |
dc.identifier.eissn | 1365-2966 | - |
dc.identifier.isi | WOS:000237783400031 | - |
dc.identifier.issnl | 0035-8711 | - |