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2021ApJ...919...99I - Astrophys. J., 919, 99-99 (2021/October-1)

Mid-infrared period-luminosity relations for Miras in the Large Magellanic Cloud.

IWANEK P., SOSZYNSKI I. and KOZLOWSKI S.

Abstract (from CDS):

We 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.

Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.

Journal keyword(s): Mira variable stars - Long period variable stars - Pulsating variable stars - Large Magellanic Cloud - Distance indicators - Stellar distance - Asymptotic giant branch stars - Carbon stars - Late-type giant stars

VizieR on-line data: <Available at CDS (J/ApJ/919/99): table3.dat>

Simbad objects: 1667

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