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dc.contributor.authorOudmaijer, R.D.
dc.contributor.authorDrew, J.E.
dc.date.accessioned2008-01-03T16:35:27Z
dc.date.available2008-01-03T16:35:27Z
dc.date.issued1999
dc.identifier.citationOudmaijer , R D & Drew , J E 1999 , ' Time-resolved spectroscopy of the peculiar H alpha variable Be star HD 76534 ' , Astronomy and Astrophysics , vol. 350 , pp. 485-490 .
dc.identifier.issn1432-0746
dc.identifier.otherdspace: 2299/1327
dc.identifier.urihttp://hdl.handle.net/2299/1327
dc.description.abstractWe present time-resolved spectroscopy of the Be star HD 76534, which was observed to have an Ha outburst in 1995, when the line went from photospheric absorption to emission at a level of more than two times the continuum within 2.5 hours. To investigate the short-term behaviour of the spectrum of HD 76534 we have obtained 30 spectra within two hours real-time and searched for variations in the spectrum.Within the levels of statistical significance, no variabilitywas found. Rather than periodic on short time scales, the H behaviour seems to be commonly episodic on longer (> 1 year) time scales, as an assessment of the existing data on theH line and the Hipparcos photometry suggests. HD 76534 underwent only 1 photometric outburst in the 3 year span that the star was monitored by the Hipparcos satellite.en
dc.format.extent208915
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.titleTime-resolved spectroscopy of the peculiar H alpha variable Be star HD 76534en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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