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dc.contributor.authorForde, K.P.
dc.contributor.authorGledhill, T.
dc.date.accessioned2012-12-11T10:29:49Z
dc.date.available2012-12-11T10:29:49Z
dc.date.issued2012-03
dc.identifier.citationForde , K P & Gledhill , T 2012 , ' Discovery of shocked H-2 around OH 231.8+4.2 ' , Monthly Notices of the Royal Astronomical Society , vol. 421 , no. 1 , pp. L49-L53 . https://doi.org/10.1111/j.1745-3933.2011.01204.x
dc.identifier.issn0035-8711
dc.identifier.otherORCID: /0000-0002-2859-4600/work/30779755
dc.identifier.urihttp://hdl.handle.net/2299/9353
dc.description.abstractWe present K-band integral field observations of the circumstellar envelope of the evolved star OH 231.8+4.2. Spatial and spectral information was simultaneously acquired using the SINFONI integral field unit, with adaptive optics, on the Very Large Telescope. The observations reveal the discovery of H-2 emission (1) around the centre of the nebula and (2) located in clumps along the western side of the northern lobe, presumably associated with the strong shocks that stimulate the previously reported H alpha emission at the same location. An observed H-2 1 -> 0/2 -> 1S(1) line ratio of 8.3 +/- 1.9 was calculated for the central field, a value consistent with shock excitation.en
dc.format.extent5
dc.format.extent360756
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleDiscovery of shocked H-2 around OH 231.8+4.2en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.date.embargoedUntil2012-10-01
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=84868135254&partnerID=8YFLogxK
rioxxterms.versionofrecord10.1111/j.1745-3933.2011.01204.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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