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Mid-infrared Period-Luminosity Relations for Miras in the Large Magellanic Cloud

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dc.abstract.enWe present the mid-infrared (mid-IR) period-luminosity relations (PLRs) using over 1000 Mira variables in the Large Magellanic Cloud, for the four Wide-field Infrared Survey Explorer and the four Spitzer bands. These PLRs cover a mid-IR wavelength range from 3.4-22 μm and are presented separately for the oxygen-rich (O-rich) and carbon-rich (C-rich) Miras. These relations can be used to measure distances to individual O-rich and/or C-rich Mira stars with an accuracy of 5% and 12%, respectively. They are the most accurate Mira PLRs in the mid-IR to date.
dc.affiliationUniwersytet Warszawski
dc.contributor.authorIwanek, Patryk
dc.contributor.authorSoszyński, Igor
dc.contributor.authorKozłowski, Szymon
dc.date.accessioned2024-01-25T11:29:38Z
dc.date.available2024-01-25T11:29:38Z
dc.date.copyright2020-12-23
dc.date.issued2021
dc.description.accesstimeBEFORE_PUBLICATION
dc.description.financeŚrodki finansowe przyznane na realizację projektu w zakresie badań naukowych lub prac rozwojowych
dc.description.number2
dc.description.versionORIGINAL_AUTHOR
dc.description.volume919
dc.identifier.doi10.3847/1538-4357/AC10C5
dc.identifier.issn0004-637X
dc.identifier.urihttps://repozytorium.uw.edu.pl//handle/item/112471
dc.identifier.weblinkhttp://adsabs.harvard.edu/abs/2021ApJ...919...99I
dc.languageeng
dc.pbn.affiliationastronomy
dc.relation.ispartofAstrophysical Journal
dc.relation.pages99
dc.rightsOther
dc.sciencecloudnosend
dc.titleMid-infrared Period-Luminosity Relations for Miras in the Large Magellanic Cloud
dc.typeJournalArticle
dspace.entity.typePublication