Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: VI: Radial abundance gradients of 29 chemical species in the Milky Way Disk
arXiv:2404.17299 · doi:10.1051/0004-6361/202450376
Abstract
Classical Cepheids (DCEPs) are crucial for calibrating the extragalactic distance ladder, ultimately enabling the determination of the Hubble constant through the PL and PW relations they exhibit. Hence it's vital to understand how the PL and PW relations depend on metallicity. This is the purpose of the C-MetaLL survey within which this work is situated. DCEPs are also very important tracers of the young populations placed along the Galactic disc. We aim to enlarge the sample of DCEPs with accurate abundances from high-resolution spectroscopy. Our goal is to extend the range of measured metallicities towards the metal-poor regime to better cover the parameter space. We observed objects in a wide range of Galactocentric radii, allowing us to study in detail the abundance gradients present in the Galactic disc. We present the results of the analysis of 331 spectra obtained for 180 individual DCEPs with a variety of high-resolution spectrographs. We derived accurate atmospheric parameters, radial velocities, and abundances for up to 29 different species. The iron abundances range between 0.5 and -1 dex with a rather homogeneous distribution in metallicity. The sample presented in this paper was complemented with that already published in the context of the C-MetaLL survey, resulting in a total of 292 pulsators whose spectra have been analysed in a homogeneous way. These data were used to study the abundance gradients of the Galactic disc in a range of Galactocentric radii spanning the range 5-20 kpc. For most of the elements we found a clear negative gradient, with a slope of -0.071\pm0.003 dex kpc^-1 for [Fe/H] case. Through a qualitative fit with the Galactic spiral arms we shown how our farthest targets (R_GC>10 kpc) trace both the Outer and OSC arms. The homogeneity of the sample will be of pivotal importance for the study of the metallicity dependance of the DCEP PL relations.
16 pages, 16 figures, 4 tables, accepted to be published in A&A, version post layout and language editor corrections
References in corpus (33)
- The Gaia mission
- Gaia Data Release 3: Summary of the content and survey properties
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- Trigonometric Parallaxes Of High-Mass Star Forming Regions: Our View Of The Milky Way
- Measurements of the Hubble Constant: Tensions in Perspective
- On the Hubble constant tension in the SNe Ia Pantheon sample
- The Zwicky Transient Facility Catalog of Periodic Variable Stars
- The mass distribution in the Galactic Centre from interferometric astrometry of multiple stellar orbits
- The influence of chemical composition on the properties of Cepheid stars. II-The iron content
- On the fine structure of the Cepheid metallicity gradient in the Galactic thin disk
- Gaia Data Release 3: Mapping the asymmetric disc of the Milky Way
- Gaia DR3: Specific processing and validation of all-sky RR Lyrae and Cepheid stars -- The Cepheid sample
- A Possible Extension of the Scutum-Centaurus Arm into the Outer Second Quadrant
- The Gaia-ESO survey: mapping the shape and evolution of the radial abundance gradients with open clusters
- The Open Cluster Chemical Abundances and Mapping Survey: VI. Galactic Chemical Gradient Analysis from APOGEE DR17
- The Galactic metallicity gradient shown by open clusters in the light of radial migration
- The ASAS-SN Catalog of Variable Stars X: Discovery of 116,000 New Variable Stars Using g-band Photometry
- Origin of neutron capture elements with the Gaia-ESO survey: the evolution of s- and r-process elements across the Milky Way
- Classical Cepheid period-Wesenheit-metallicity relation in the Gaia bands
- An updated metal-dependent theoretical scenario for Classical Cepheids
- Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: I. HARPS-N@TNG spectroscopy of 47 Classical Cepheid and 1 BL Her variables
- Tracing the Milky Way warp and spiral arms with classical Cepheids
- Radial Migration from Metallicity Gradient of Open Clusters and Outliers
- Using classical Cepheids to study the far side of the Milky Way disk: I. Spectroscopic classification and the metallicity gradient
- Oxygen, sulfur, and iron radial abundance gradients of classical Cepheids across the Galactic thin disk
- Study of changes in the pulsation period of 148 Galactic Cepheid variables
- Period-Age-Metallicity and Period-Age-Color-Metallicity relations for Classical Cepheids: an application to the Gaia EDR3 sample
- Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: II.High-resolution spectroscopy of the most metal poor Galactic Cepheids
- Using classical Cepheids to study the far side of the Milky Way disk. II. The spiral structure in the first and fourth Galactic quadrants
- Updated theoretical Period-Age and Period-Age-Color relations for Galactic Classical Cepheids: an application to the Gaia DR2 sample
- Analytic solution of Chemical Evolution Models with Type Ia SNe
- The Gaia-ESO Survey: Chemical tagging in the thin disk. Open clusters blindly recovered in the elemental abundance space
- Type II and anomalous Cepheids in the Kepler K2 mission
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- The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision
- Mapping radial abundance gradients with Gaia-ESO open clusters: Evidence of recent gas accretion in the Milky Way disk
- Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift
- MAGIS (Measuring Abundances of red super Giants with Infrared Spectroscopy) project I. Establishment of an abundance analysis procedure for red supergiants and its evaluation with nearby stars
- Toward a Comprehensive Grid of Cepheid Models with MESA II. Impact of Physical and Numerical Assumptions on Elemental Abundances
- Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: IX. Metallicity dependence of Period-Wesenheit relations based on a homogeneous spectroscopic sample
- Cepheid Metallicity in the Leavitt Law (C--MetaLL) survey: VIII. High-Resolution IGRINS Spectroscopy of 23 Classical Cepheids: Validating NIR Abundances
- Near-IR CO and CN in classical Cepheids
- A hybrid SLAM-Payne framework for atmospheric parameter and abundance determination of early-type Stars from LAMOST DR9 low-resolution Spectra