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dc.contributor.authorGatti, A.A.
dc.contributor.authorDrew, J.E.
dc.contributor.authorLumsden, S.
dc.contributor.authorMarsh, T.R.
dc.contributor.authorMoran, C.
dc.contributor.authorStetson, P.
dc.date.accessioned2009-12-01T13:27:22Z
dc.date.available2009-12-01T13:27:22Z
dc.date.issued1997
dc.identifier.citationGatti , A A , Drew , J E , Lumsden , S , Marsh , T R , Moran , C & Stetson , P 1997 , ' A radial velocity study of the companion to the central star of Abell 35 ' Monthly Notices of the Royal Astronomical Society , vol. 291 , no. 4 , pp. 773-779 .
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 155700
dc.identifier.otherPURE UUID: c0bc0f65-d743-4c7d-b20f-1cb765c5bd86
dc.identifier.otherdspace: 2299/4037
dc.identifier.otherScopus: 0039832656
dc.identifier.urihttp://hdl.handle.net/2299/4037
dc.descriptionOriginal article can be found at: http://adsabs.harvard.edu/basic_search.html Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractWe report the results of a radial velocity study of BD - 22.3467 deg (LW Hya), the cool companion to the subdwarf central star of the planetary nebula Abell 35. Estimates for its radial velocity have been obtained by cross correlation with radial velocity standards for five epochs of observations sampling periods of the order of days and decades. We find that any radial velocity variation of BD - 22.3467 deg on periods shorter than 30 d cannot possess a semi-amplitude greater than 5 km/s. Also, with the exception of a limited number of possible periods not covered by our sampling frequency, we can exclude radial velocity variations of semi-amplitude larger than about 8 km/s up to periods of approximately 30 yr. On the other hand, short-period, small-semi-amplitude about 5 km/s) radial velocity variations have been observed in the blue spectral region and possibly, with a smaller semi-amplitude (about 2 km/s), in the red. The photometric period of 0.766 +/- 0.001 d, which has been associated with the rotation of the star, is consistent with them, although other periods cannot yet be ruled out.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectplanetary nebulae
dc.subjectbinary
dc.titleA radial velocity study of the companion to the central star of Abell 35en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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