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dc.contributor.authorArai, A.
dc.contributor.authorIsogai, M.
dc.contributor.authorYamanaka, M.
dc.contributor.authorAkitaya, H.
dc.contributor.authorUemura, M.
dc.date.accessioned2023-01-18T14:27:10Z
dc.date.available2023-01-18T14:27:10Z
dc.date.issued2015
dc.identifier.citationActa Polytechnica. 2015, vol. 2, no. 1, p. 257-260.
dc.identifier.issn1210-2709 (print)
dc.identifier.issn1805-2363 (online)
dc.identifier.urihttp://hdl.handle.net/10467/105795
dc.description.abstractWe report on the results of our low resolution spectroscopic observations during the 2011 outburst of the recurrent nova T Pyx. Our observations were performed from 0.19 days to 34 days after the eruption discovered by M. Linnolt. We found Wolf-Rayet like features in our spectrum during the initial rising phase on t = 0.19 d. Following spectral developments are consistent with previous works. We discuss that the early phase of T Pyx is divided into three stages, a short lived WR-like stage, He/N stage and Fe II stage.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherČeské vysoké učení technické v Prazecs
dc.publisherCzech Technical University in Pragueen
dc.relation.ispartofseriesActa Polytechnica
dc.relation.urihttps://ojs.cvut.cz/ojs/index.php/APP/article/view/2915
dc.rightsCreative Commons Attribution 4.0 International Licenseen
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.titleOptical Low Resolution Spectroscopic Observations of T Pyx during the Early Phase of 2011 Outburst
dc.typearticleen
dc.date.updated2023-01-18T14:27:10Z
dc.identifier.doi10.14311/APP.2015.02.0257
dc.rights.accessopenAccess
dc.type.statusPeer-reviewed
dc.type.versionpublishedVersion


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Creative Commons Attribution 4.0 International License
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