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Galactic calibration of the tip of the red giant branch

Mould, Jeremy; Clementini, G; Da Costa, Gary

Description

Indications from Gaia data release 2 are that the tip of the red giant branch (a population II standard candle related to the helium flash in low mass stars) is close to -4 in absolute I magnitude in the Cousins photometric system. Our sample is high-latitude southern stars from the thick disk and inner halo, and our result is consistent with longstanding findings from globular clusters, whose distances were calibrated with RR Lyrae stars. As the Gaia mission proceeds, there is every reason to...[Show more]

dc.contributor.authorMould, Jeremy
dc.contributor.authorClementini, G
dc.contributor.authorDa Costa, Gary
dc.date.accessioned2022-05-03T01:34:57Z
dc.identifier.issn1448-6083
dc.identifier.urihttp://hdl.handle.net/1885/264248
dc.description.abstractIndications from Gaia data release 2 are that the tip of the red giant branch (a population II standard candle related to the helium flash in low mass stars) is close to -4 in absolute I magnitude in the Cousins photometric system. Our sample is high-latitude southern stars from the thick disk and inner halo, and our result is consistent with longstanding findings from globular clusters, whose distances were calibrated with RR Lyrae stars. As the Gaia mission proceeds, there is every reason to think an accurate Galactic geometric calibration of tip of the red giant branch will be a significant outcome for the extragalactic distance scale.
dc.description.sponsorshipParts of this project were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020
dc.format.mimetypeapplication/pdf
dc.language.isoen_AU
dc.publisherCommonwealth Scientific and Industrial Research Organization Publishing
dc.rights© Astronomical Society of Australia 2019; published by Cambridge University Press
dc.sourcePublications of the Astronomical Society of Australia
dc.subjectparallax, stars
dc.subjectred giants, galaxies: distances and redshifts
dc.titleGalactic calibration of the tip of the red giant branch
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume36
dc.date.issued2019
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu3102795xPUB2299
local.publisher.urlhttp://journals.cambridge.org/action/displayJournal?jid=PAS
local.type.statusAccepted Version
local.contributor.affiliationMould, Jeremy, Swinburne University
local.contributor.affiliationClementini, G, INAF, Osservatorio Astronomico di Bologna
local.contributor.affiliationDa Costa, Gary, College of Science, ANU
dc.relationhttp://purl.org/au-research/grants/arc/CE1101020
local.bibliographicCitation.startpage1
local.bibliographicCitation.lastpage6
local.identifier.doi10.1017/pasa.2018.46
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
dc.date.updated2020-12-27T07:24:19Z
local.identifier.thomsonID4.55364E+11
dcterms.accessRightsOpen Access
dcterms.provenancehttps://v2.sherpa.ac.uk/id/publication/7759..."The Accepted Version can be archived in a Non-Commercial Institutional Repository. 6 months embargo" from SHERPA/RoMEO site (as at 27/05/2022).
CollectionsANU Research Publications

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