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Conference Paper: A homogeneous distance catalogue for Galactic RV Tauri objects

TitleA homogeneous distance catalogue for Galactic RV Tauri objects
Authors
Vicker, SBFrew, DJOwers, MSParker, QABojicic, I
Issue Date2016
PublisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU
Citation
Proceedings of the International Astronomical Union Symposium 323 (IAUS323): Planetary Nebulae: Multi-Wavelength Probes of Stellar and Galactic Evolution, Beijing, China, 10-14 October 2016, v. 12 n. S323, p. 371-372 How to Cite?
DOI: http://dx.doi.org/10.1017/S1743921317000606
AbstractA subset of Post-AGB (PAGB) objects are the highly luminous RV Tauri variables that show similarities to Type-II Cepheids. By using a sample of known RV Tauri stars from the Magellanic Clouds we are able to determine period luminosity relationships (PLRs) in various bands that have been used to determine the luminosities of their Galactic counterparts. We have gathered all available photometry in order to generate an SED for each object and determine the total integrated flux. This total flux combined with a calculated or inferred intrinsic luminosity leads to a distance (Vickers et al. 2015). This distance catalogue has allowed us to begin to constrain the physical parameters of this poorly understood evolutionary phase and to determine links between these physical characteristics as a function of their stellar population.
Persistent Identifierhttp://hdl.handle.net/10722/256484
ISBN
9781107169913
ISSN
1743-9213
2023 SCImago Journal Rankings: 0.121
ISI Accession Number ID
WOS:000456283100076
Series/Report no.Proceedings of the International Astronomical Union Symposia and Colloquia

 

DC FieldValueLanguage
dc.contributor.authorVicker, SB-
dc.contributor.authorFrew, DJ-
dc.contributor.authorOwers, MS-
dc.contributor.authorParker, QA-
dc.contributor.authorBojicic, I-
dc.date.accessioned2018-07-20T06:35:24Z-
dc.date.available2018-07-20T06:35:24Z-
dc.date.issued2016-
dc.identifier.citationProceedings of the International Astronomical Union Symposium 323 (IAUS323): Planetary Nebulae: Multi-Wavelength Probes of Stellar and Galactic Evolution, Beijing, China, 10-14 October 2016, v. 12 n. S323, p. 371-372-
dc.identifier.isbn9781107169913-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/10722/256484-
dc.description.abstractA subset of Post-AGB (PAGB) objects are the highly luminous RV Tauri variables that show similarities to Type-II Cepheids. By using a sample of known RV Tauri stars from the Magellanic Clouds we are able to determine period luminosity relationships (PLRs) in various bands that have been used to determine the luminosities of their Galactic counterparts. We have gathered all available photometry in order to generate an SED for each object and determine the total integrated flux. This total flux combined with a calculated or inferred intrinsic luminosity leads to a distance (Vickers et al. 2015). This distance catalogue has allowed us to begin to constrain the physical parameters of this poorly understood evolutionary phase and to determine links between these physical characteristics as a function of their stellar population.-
dc.languageeng-
dc.publisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU-
dc.relation.ispartofProceedings of the International Astronomical Union-
dc.relation.ispartofseriesProceedings of the International Astronomical Union Symposia and Colloquia-
dc.rightsProceedings of the International Astronomical Union. Copyright © Cambridge University Press.-
dc.titleA homogeneous distance catalogue for Galactic RV Tauri objects-
dc.typeConference_Paper-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityFrew, DJ=rp02013-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.authorityBojicic, I=rp02020-
dc.identifier.doi10.1017/S1743921317000606-
dc.identifier.hkuros286287-
dc.identifier.hkuros286281-
dc.identifier.volume12-
dc.identifier.issueS323-
dc.identifier.spage371-
dc.identifier.epage372-
dc.identifier.isiWOS:000456283100076-
dc.publisher.placeUnited Kingdom-
dc.identifier.issnl1743-9213-

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