The panchromatic view of the Magellanic Clouds from Classical Cepheids. I. Distance, Reddening and Geometry of the Large Magellanic Cloud disk

Abstract

We present a detailed investigation of the Large Magellanic Cloud (LMC) disk using classical Cepheids. Our analysis is based on optical (I,V; OGLE-IV), near-infrared (NIR: J,H,Ks) and mid-infrared (MIR: w1; WISE) mean magnitudes. By adopting new templates to estimate the NIR mean magnitudes from single-epoch measurements, we build the currently most accurate, largest and homogeneous multi-band dataset of LMC Cepheids. We determine Cepheid individual distances using optical and NIR Period-Wesenheit relations (PWRs), to measure the geometry of the LMC disk and its viewing angles. Cepheid distances based on optical PWRs are precise at 3%, but accurate to 7, while the ones based on NIR PWRs are more accurate (to 3%), but less precise (2%-15%), given the higher photometric error on the observed magnitudes. We found an inclination i=25.05 $\pm$ 0.02 (stat.) $\pm$ 0.55 (syst.) deg, and a position angle of the lines of nodes P.A.=150.76 $\pm$ 0.02(stat.) $\pm$ 0.07(syst.) deg. These values agree well with estimates based either on young (Red Supergiants) or on intermediate-age (Asymptotic Giant Branch, Red Clump) stellar tracers, but they significantly differ from evaluations based on old (RR Lyrae) stellar tracers. This indicates that young/intermediate and old stellar populations have different spatial distributions. Finally, by using the reddening-law fitting approach, we provide a reddening map of the LMC disk which is ten times more accurate and two times larger than similar maps in the literature. We also found an LMC true distance modulus of ${\mu }_{0,LMC}=18.48\pm 0.10$ (stat. and syst.) mag, in excellent agreement with the currently most accurate measurement (Pietrzynski et al. 2013).

arXiv comment24 pages, 15 figures, to be published in ApJ

References in corpus (51)

• Color Transformations for the 2MASS Second Incremental Data Release
• The MACHO Project: Microlensing Results from 5.7 Years of LMC Observations
• An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent
• Are the Magellanic Clouds on their First Passage about the Milky Way?
• Third-Epoch Magellanic Cloud Proper Motions I: HST/WFC3 data and Orbit Implications
• Magellanic Cloud Structure from Near-IR Surveys I: The Viewing Angles of the LMC
• Hubble Space Telescope Fine Guidance Sensor Parallaxes of Galactic Cepheid Variable Stars: Period-Luminosity Relations
• The Role of Dwarf Galaxy Interactions in Shaping the Magellanic System and Implications for Magellanic Irregulars
• The VMC Survey - I. Strategy and First Data
• Third-Epoch Magellanic Cloud Proper Motions II: The Large Magellanic Cloud Rotation Field in Three Dimensions
• A new calibration of Galactic Cepheid Period-Luminosity relations from B to K bands, and a comparison to LMC PL relations
• The influence of chemical composition on the properties of Cepheid stars. II-The iron content
• Cepheid Parallaxes and the Hubble Constant
• The Tidal Origin of the Magellanic Stream and the Possibility of a Stellar Counterpart
• Cepheid Period-Radius and Period-Luminosity Relations and the Distance to the LMC
• New Optical Reddening Maps of the Large and Small Magellanic Clouds
• Magellanic Cloud Structure from Near-IR Surveys II: Star Count Maps and the Intrinsic Elongation of the LMC
• Insights into the Cepheid distance scale
• A Population of Accreted SMC Stars in the LMC
• Theoretical Models for Classical Cepheids: II. Period-Luminosity, Period-Color and Period-Luminosity-Color Relations
• Classical Cepheid Pulsation Models. III. The Predictable Scenario
• Cepheid pulsation models at varying metallicity and DY/DZ
• Structure of the Large Magellanic Cloud from 2MASS
• The VMC Survey IV. The LMC star formation history and disk geometry from four VMC tiles
• Calibrating the Cepheid Period-Luminosity relation from the infrared surface brightness technique II. The effect of metallicity, and the distance to the LMC
• Large Magellanic Cloud Near-Infrared Synoptic Survey. I. Cepheid variables and the calibration of the Leavitt Law
• The Carina Project: II. Stellar Populations
• First Results from the NOAO Survey of the Outer Limits of the Magellanic Clouds
• On the distance of the Magellanic Clouds using Cepheid NIR and optical-NIR Period Wesenheit Relations
• Mean JHK Magnitudes of Fundamental-Mode Cepheids from Single-Epoch Observations
• The VMC Survey. V. First results for Classical Cepheids
• Constraining the orbital history of the Magellanic Clouds: A new bound scenario suggested by the tidal origin of the Magellanic Stream
• Kinematic Evidence for an Old Stellar Halo in the Large Magellanic Cloud
• Cepheid theoretical models and observations in HST/WFC3 filters: the effect on the Hubble constant Ho
• Galactic Cepheids with Spitzer: I. Leavitt Law and Colors
• Three dimensional maps of the Magellanic Clouds using RR~Lyrae stars and Cepheids - I. The Large Magellanic Cloud
• The Eclipsing Binary Cepheid OGLE-LMC-CEP-0227 in the Large Magellanic Cloud: pulsation modelling of light and radial velocity curves
• New NIR light-curve templates for classical Cepheids
• Hubble Tarantula Treasury Project. IV. The extinction law
• Metallicities, Age--Metallicity relationships, and Kinematics of Red Giant Branch Stars in the Outer Disk of the Large Magellanic Cloud
• On the distance of Magellanic Clouds: first overtone Cepheids
• Structure of the Large Magellanic Cloud from the Near Infrared magnitudes of Red Clump stars
• Surface Brightness and Stellar Populations at the Outer Edge of the Large Magellanic Cloud: No Stellar Halo Yet
• A New Cepheid Distance Measurement and Method for NGC 6822
• The Carina Project. VIII. The α-element abundances
• The Carina Project. IV. radial velocity distribution
• Recent Star Formation in the Leading Arm of the Magellanic Stream
• The Detailed Forms of the LMC Cepheid PL and PLC Relations
• Chemical and structural analysis of the Large Magellanic Cloud using the fundamental mode RR Lyrae stars
• H I Kinematics of the Large Magellanic Cloud revisited : Evidence of possible infall and outflow
• Theoretical Cepheid Period-Luminosity And Period-Color Relations In Spitzer IRAC Bands

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• Peeping into recent star formation history of the Magellanic Clouds
• The VMC survey -- XLVI. Stellar proper motions in the centre of the Large Magellanic Cloud
• Variable stars in the Gaia era: Mira, RR Lyrae, delta and Type-II Cepheids