Large Magellanic Cloud Near-Infrared Synoptic Survey. IV. Leavitt Laws for Type II Cepheid Variables

Abstract

We present time-series observations of Population \rom{2} Cepheids in the Large Magellanic Cloud at near-infrared ($JH{K}_s$) wavelengths. Our sample consists of 81 variables with accurate periods and optical ($VI$) magnitudes from the OGLE survey, covering various subtypes of pulsators (BL Herculis, W Virginis and RV Tauri). We generate light curve templates using high-quality $I$-band data in the LMC from OGLE and $K_s$-band data in the Galactic Bulge from VVV and use them to obtain robust mean magnitudes. We derive Period-Luminosity (P-L) relations in the near-infrared and Period-Wesenheit (P-W) relations by combining optical and near-infrared data. Our P-L and P-W relations are consistent with published work when excluding long-period RV Tauris. We find that Pop II Cepheids and RR Lyraes follow the same P-L relations in the LMC. Therefore, we use trigonometric parallax from the {\it Gaia DR1} for VY~Pyx and the {\it Hubble Space Telescope} parallaxes for $k$~Pav and 5 RR Lyrae variables to obtain an absolute calibration of the Galactic $K_s$-band P-L relation, resulting in a distance modulus to the LMC of ${\mu }_{\mathrm{LMC}}=18.54\pm 0.08$~mag. We update the mean magnitudes of Pop~II Cepheids in Galactic globular clusters using our light curve templates and obtain distance estimates to those systems, anchored to a precise late-type eclipsing binary distance to the LMC. We find the distances to these globular clusters based on Pop~II Cepheids are consistent (within $2\sigma$) with estimates based on the $M_V-[\mathrm{Fe}/\mathrm{H}]$ relation for horizontal branch stars.

arXiv commentAccepted for publication in The Astronomical Journal

References in corpus (26)

• Validation of the new Hipparcos reduction
• A 2.4% Determination of the Local Value of the Hubble Constant
• VISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way
• An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent
• Gaia Data Release 1: Astrometry - one billion positions, two million proper motions and parallaxes
• The VMC Survey - I. Strategy and First Data
• Clustering of Local Group distances: publication bias or correlated measurements? I. The Large Magellanic Cloud
• New Optical Reddening Maps of the Large and Small Magellanic Clouds
• The Luminosities and Distance Scales of Type II Cepheid and RR Lyrae variables
• Distance Scale Zero-Points from Galactic RR Lyrae Star Parallaxes
• The distance to the Galactic Centre based on Population-II Cepheids and RR Lyrae stars
• The RR Lyrae Period - K Luminosity relation for Globular Clusters: an observational approach
• The MACHO Project LMC Variable Star Inventory: The Discovery of RV Tauri stars and New Type II Cepheids in the LMC
• Large Magellanic Cloud Near-Infrared Synoptic Survey. I. Cepheid variables and the calibration of the Leavitt Law
• The period-luminosity relation for type II Cepheids in globular clusters
• The Carnegie Hubble Program: The Leavitt Law at 3.6 and 4.5 micron in the Milky Way
• Mean JHK Magnitudes of Fundamental-Mode Cepheids from Single-Epoch Observations
• New near-infrared period-luminosity-metallicity relations for RR Lyrae stars and the outlook for Gaia
• The VMC Survey. XIII. Type II Cepheids in the Large Magellanic Cloud
• New NIR light-curve templates for classical Cepheids
• Large Magellanic Cloud Near-Infrared Synoptic Survey. II. The Wesenheit relations and their application to the Distance scale
• Period-luminosity relations of type II Cepheids in the Magellanic Clouds
• Period-Luminosity Relations for Type II Cepheids and their Application
• On the Variation of Fourier Parameters for Galactic and LMC Cepheids at Optical, Near-Infrared and Mid-Infrared Wavelengths
• Large Magellanic Cloud Near-Infrared Synoptic Survey. III. A Statistical Study of Non-Linearity in the Leavitt Laws
• A Comparative Study of Multiwavelength Theoretical and Observed Light Curves of Cepheid Variables

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