Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/23443
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Rosenfield, P. | en_US |
dc.contributor.author | Marigo, P. | en_US |
dc.contributor.author | GIRARDI, Leo Alberto | en_US |
dc.contributor.author | Dalcanton, J. J. | en_US |
dc.contributor.author | Bressan, A. | en_US |
dc.contributor.author | GULLIEUSZIK, MARCO | en_US |
dc.contributor.author | Weisz, D. R. | en_US |
dc.contributor.author | Williams, B. F. | en_US |
dc.contributor.author | Dolphin, A. | en_US |
dc.contributor.author | Aringer, B. | en_US |
dc.date.accessioned | 2020-03-20T16:46:28Z | - |
dc.date.available | 2020-03-20T16:46:28Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.isbn | 978-1-58381-878-7 | en_US |
dc.identifier.issn | 1050-3390 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/23443 | - |
dc.description.abstract | The evolution and lifetimes of thermally pulsing asymptotic giant branch (TP-AGB) stars suffer from significant uncertainties. We present a detailed framework for constraining model luminosity functions of TP-AGB stars using resolved stellar populations. We show an example of this method that compares various TP-AGB mass-loss prescriptions that differ in their treatments of mass loss before the onset of dust-driven winds (pre-dust). We find that models with more efficient pre-dust driven mass loss produce results consistent with observations, as opposed to more canonical mass-loss models. Efficient pre-dust driven mass-loss predicts, for [Fe/H] ≲ -1.2, that lower mass TP-AGB stars (M≲ 1 M<SUB>☉</SUB>) must have lifetimes less than about 1.2 Myr. | en_US |
dc.language.iso | eng | en_US |
dc.title | Constraining Mass Loss and Lifetimes of Low Mass, Low Metallicity AGB Stars | en_US |
dc.type | Conference paper | - |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 497 | en_US |
dc.relation.firstpage | 423 | en_US |
dc.type.referee | REF_0 | en_US |
dc.relation.alleditors | Kerschbaum, F.; Wing, R. F.; Hron, J. | en_US |
dc.relation.ispartofbook | Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | Why Galaxies Care About AGB Stars III | en_US |
dc.relation.conferenceplace | Vienna | en_US |
dc.relation.conferencedate | July 28 - August 1, 2014 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES | en_US |
dc.identifier.adsbibcode | 2015ASPC..497..423R | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0002-6301-3269 | - |
crisitem.author.orcid | 0000-0002-7296-9780 | - |
crisitem.journal.journalissn | 1050-3390 | - |
crisitem.journal.ance | E210915 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
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