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dc.contributor.authorKepler, Souza Oliveirapt_BR
dc.contributor.authorFraga, Lucianopt_BR
dc.contributor.authorWinget, Donald Earlpt_BR
dc.contributor.authorBell, Keatonpt_BR
dc.contributor.authorCórsico, Alejandro Hugopt_BR
dc.contributor.authorWerner, Klauspt_BR
dc.date.accessioned2014-11-15T02:15:56Zpt_BR
dc.date.issued2014pt_BR
dc.identifier.issn0035-8711pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/106995pt_BR
dc.description.abstractWe report the discovery of pulsations in the spectroscopic PG 1159 type pre-white dwarf SDSS J075415.12 + 085232.18. Analysis of the spectrum by Werner et al. indicated Teff = 120 000 ± 10 000 K, log g = 7.0 ± 0.3, mass M= 0.52 ± 0.02Mʘ, C/He = 0.33 by number. We obtained time series images with the SOAR 4.1 m telescope and 2.1 m Otto Struve telescope at McDonald Observatory and show the star is also a variable PG 1159 type star, with dominant period of 525 s.en
dc.format.mimetypeapplication/pdf
dc.language.isoengpt_BR
dc.relation.ispartofMonthly notices of the Royal Astronomical Society. Oxford. Vol. 442, no. 3 (Aug. 2014), p. 2278–2281pt_BR
dc.rightsOpen Accessen
dc.subjectStars: individual: SDSS J075415.12 + 085232.18en
dc.subjectAnãs brancaspt_BR
dc.subjectWhite dwarfsen
dc.titleDiscovery of a new PG 1159 (GW Vir) pulsatorpt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000942394pt_BR
dc.type.originEstrangeiropt_BR


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