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dc.contributor.authorBurningham, B.
dc.contributor.authorNaylor, T.
dc.contributor.authorLittlefair, S.P.
dc.contributor.authorJefferies, R.D.
dc.date.accessioned2011-06-22T07:19:23Z
dc.date.available2011-06-22T07:19:23Z
dc.date.issued2005
dc.identifier.citationBurningham , B , Naylor , T , Littlefair , S P & Jefferies , R D 2005 , Estimating the low-mass IMF in OB associations : o Orionis . in The Initial Mass Function 50 Years Later . Astrophysics and Space Science Library , no. III , vol. 327 , Springer Nature , pp. 141-142 . https://doi.org/10.1007/978-1-4020-3407-7_24
dc.identifier.isbn978-1-4020-3406-0
dc.identifier.isbn978-1-4020-3407-7
dc.identifier.otherPURE: 167566
dc.identifier.otherPURE UUID: 347dd93b-a8b1-41a5-8a56-8c5d0b2e70d5
dc.identifier.otherdspace: 2299/6037
dc.identifier.otherORCID: /0000-0003-4600-5627/work/64327336
dc.identifier.urihttp://hdl.handle.net/2299/6037
dc.description“The original publication is available at www.springerlink.com” Copyright Springer [Full text of this chapter is not available in the UHRA]
dc.description.abstractWe investigate the issues of contamination and exclusion in photometric membership selection techniques when applied to OB associations. We use radial velocities to calculate membership probabilities for a sample of very low-mass candidate members of the σ Orionis young group. We find that significant numbers of bona members are not excluded by photometric selection techniques, and for I brighter than 17 there is not significant contamination in the expected PMS region.en
dc.language.isoeng
dc.publisherSpringer Nature
dc.relation.ispartofThe Initial Mass Function 50 Years Later
dc.relation.ispartofseriesAstrophysics and Space Science Library
dc.titleEstimating the low-mass IMF in OB associations : o Orionisen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
rioxxterms.versionofrecordhttps://doi.org/10.1007/978-1-4020-3407-7_24
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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