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- Publisher Website: 10.1111/j.1365-2966.2005.08684.x
- Scopus: eid_2-s2.0-15244354216
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Article: A circular planetary nebula around the OH/IR star OH 354.88-0.54 (V1018 Sco)
Title | A circular planetary nebula around the OH/IR star OH 354.88-0.54 (V1018 Sco) |
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Authors | |
Keywords | Stars: AGB and post-AGB Planetary nebulae: General Masers |
Issue Date | 2005 |
Citation | Monthly Notices of the Royal Astronomical Society, 2005, v. 357, n. 4, p. 1189-1196 How to Cite? |
Abstract | New deep, high-resolution Ha imagery from the UK Schmidt Telescope (UKST) Unit's Ha survey of the Southern Galactic Plane reveals the presence of a faint, highly circular, planetary nebula (PN) surrounding a very long-period variable star (now known as V1018 Sco), first discovered as a 1612-MHz OH maser, OH 354.88-0.54. The nebular phase-lag distance, diameter and radial velocity are 3.2 kpc, 0.3 pc and 13 km s -1, respectively. Combining the maser attributes with near-, mid- and far-infrared data and with our optical spectrum of the ring we conclude that the object was an intermediate-mass asymptotic giant branch (AGB) star (initial stellar mass ≥ 4M⊙) in which the fast wind has recently turned on, ionizing previously shed circumstellar material. Hence, we speculate that we may be witnessing a hitherto unobserved phase of PN evolution, in which a PN has only recently started to form around a star that is unequivocally still in its AGB phase. © 2005 RAS. |
Persistent Identifier | http://hdl.handle.net/10722/208834 |
ISSN | 2021 Impact Factor: 5.235 2020 SCImago Journal Rankings: 2.058 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Cohen, Martin G. | - |
dc.contributor.author | Parker, Quentin A. | - |
dc.contributor.author | Chapman, Jessica M. | - |
dc.date.accessioned | 2015-03-23T02:01:51Z | - |
dc.date.available | 2015-03-23T02:01:51Z | - |
dc.date.issued | 2005 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, 2005, v. 357, n. 4, p. 1189-1196 | - |
dc.identifier.issn | 0035-8711 | - |
dc.identifier.uri | http://hdl.handle.net/10722/208834 | - |
dc.description.abstract | New deep, high-resolution Ha imagery from the UK Schmidt Telescope (UKST) Unit's Ha survey of the Southern Galactic Plane reveals the presence of a faint, highly circular, planetary nebula (PN) surrounding a very long-period variable star (now known as V1018 Sco), first discovered as a 1612-MHz OH maser, OH 354.88-0.54. The nebular phase-lag distance, diameter and radial velocity are 3.2 kpc, 0.3 pc and 13 km s -1, respectively. Combining the maser attributes with near-, mid- and far-infrared data and with our optical spectrum of the ring we conclude that the object was an intermediate-mass asymptotic giant branch (AGB) star (initial stellar mass ≥ 4M⊙) in which the fast wind has recently turned on, ionizing previously shed circumstellar material. Hence, we speculate that we may be witnessing a hitherto unobserved phase of PN evolution, in which a PN has only recently started to form around a star that is unequivocally still in its AGB phase. © 2005 RAS. | - |
dc.language | eng | - |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | - |
dc.subject | Stars: AGB and post-AGB | - |
dc.subject | Planetary nebulae: General | - |
dc.subject | Masers | - |
dc.title | A circular planetary nebula around the OH/IR star OH 354.88-0.54 (V1018 Sco) | - |
dc.type | Article | - |
dc.description.nature | link_to_OA_fulltext | - |
dc.identifier.doi | 10.1111/j.1365-2966.2005.08684.x | - |
dc.identifier.scopus | eid_2-s2.0-15244354216 | - |
dc.identifier.volume | 357 | - |
dc.identifier.issue | 4 | - |
dc.identifier.spage | 1189 | - |
dc.identifier.epage | 1196 | - |
dc.identifier.isi | WOS:000227349800008 | - |
dc.identifier.issnl | 0035-8711 | - |