Imagen de Portada

Using a neural network approach and starspots dependent models to predict effective temperatures and ages of young stars

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Tarantino, Marco, Prisinzano, Loredana, Angelo, Nicoletta D, Damiani, Francesco, Adelfio, Giada
Formato:	Preprint
Publicado:	2025
Materias:	Solar and Stellar Astrophysics Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Asteroseismic ages for 17,000 stars in Kepler, K2 and TESS
por: Willett, Emma, et al.
Publicado: (2026)

The age and metallicity dependence of the near-infrared absolute magnitude and colour of red clump stars
por: Onozato, Hiroki, et al.
Publicado: (2025)

Spectral classification of young stars using conditional invertible neural networks II. Application to Trumpler 14 in Carina
por: Kang, Da Eun, et al.
Publicado: (2025)

Centrally concentrated star formation in young clusters
por: Assilkhan, Adilkhan, et al.
Publicado: (2025)

Exploring the dependence of chemical traits on metallicity: chemical trends for red giant stars with asteroseismic ages
por: Vitali, S., et al.
Publicado: (2024)

Properties of intermediate- to high-mass stars in the young cluster M17 -- Characterizing the (pre-)zero-age main sequence
por: Backs, Frank, et al.
Publicado: (2024)

A neural network approach to determining photometric metallicities of M-type dwarf stars
por: Duque-Arribas, C., et al.
Publicado: (2025)

The population of young low-mass stars in Trumpler 14
por: Itrich, Dominika, et al.
Publicado: (2023)

Using detailed single star and binary evolution models to probe the large observed luminosity spread of red supergiants in young open star clusters
por: Wang, Chen, et al.
Publicado: (2025)

The Gaia-ESO Survey: 3D dynamics of young groups and clusters from GES and Gaia EDR3
por: Wright, Nicholas J., et al.
Publicado: (2023)

Atmospheric parameters and chemical abundances of young stars with APOGEE. I. Orion star-forming region
por: López-Valdivia, Ricardo, et al.
Publicado: (2025)

Massive extended streamers feed high-mass young stars
por: Olguin, Fernando A., et al.
Publicado: (2025)

The effect of the environment-dependent stellar initial mass function on the photometric properties of star-forming galaxies
por: Haslbauer, Moritz, et al.
Publicado: (2024)

The age sequence of young clusters in Perseus: Estimating ages from mass distributions
por: Pavlidou, Tatiana, et al.
Publicado: (2026)

Dynamical traceback age of the Octans young stellar association
por: Galli, P. A. B., et al.
Publicado: (2024)

VLBI detection of nearby (< 100 pc) young stars: Pilot observations
por: Dzib, Sergio A., et al.
Publicado: (2024)

Most nearby young star clusters formed in three massive complexes
por: Swiggum, Cameren, et al.
Publicado: (2024)

The variable stars population of the extended young globular cluster NGC 1851
por: Ferro, A. Arellano, et al.
Publicado: (2024)

Hadronic acceleration in the young star cluster NGC 6611 inside the M16 region unveiled by Fermi-LAT: constraints on the acceleration efficiency
por: Peron, Giada, et al.
Publicado: (2025)

Calibration of the JAGB method for the Magellanic Clouds and Milky Way from Gaia DR3, considering the role of oxygen-rich AGB stars
por: Magnus, Else, et al.
Publicado: (2024)

Evolution of stars with 60 and 200 Msun: predictions for WNh stars in the Milky Way
por: Gormaz-Matamala, Alex Camilo, et al.
Publicado: (2024)

At the same age, metallicity, and alpha-enhancement, sodium is a more effective tracer of the young and old sequences of the Milky Way disc
por: Owusu, Evans K., et al.
Publicado: (2024)

Molecular inventory of a young eruptive star's environment -- Case study of the classical FU Orionis star V1057 Cyg
por: Szabó, Zs. M., et al.
Publicado: (2025)

EWOCS-III: JWST observations of the supermassive star cluster Westerlund 1
por: Guarcello, M. G., et al.
Publicado: (2024)

Stellar population astrophysics (SPA) with the TNG. Abundance analysis of nearby red giants and red clump stars: combining high resolution spectroscopy and asteroseismology
por: Vernekar, Nagaraj, et al.
Publicado: (2024)

Dynamical masses of young stellar objects with the VLBA: DYNAMO-VLBA: Radio binary stars in Orion
por: Dzib, Sergio A., et al.
Publicado: (2026)

Testing stellar yield prescriptions in OMEGA+: Implications for rising sodium abundances in young thick disc stars
por: Owusu, Evans K., et al.
Publicado: (2025)

The GRAVITY young stellar object survey XII. The hot gas disk component in Herbig Ae/Be stars
por: GRAVITY Collaboration, et al.
Publicado: (2024)

Bayesian ages of local young stellar associations I. Through the expansion rate method
por: Olivares, J., et al.
Publicado: (2025)

Obscured star clusters in the Inner Milky Way. How many massive young clusters are still awaiting detection?
por: Gupta, Akash, et al.
Publicado: (2024)

Unveiling very young O stars. Two Galactic O2V((f*))z in Westerlund 2
por: Roman-Lopes, A.
Publicado: (2024)

The arc-shaped radio source at the center of NGC 6334A: Is it a colliding wind region of two young massive stars or the bow shock of a runaway star?
por: Yanza, Vanessa, et al.
Publicado: (2025)

New parameters for star cluster dynamics: observational results
por: Lanzoni, Barbara, et al.
Publicado: (2026)

The age of the Methuselah star in light of stellar evolution models with tailored abundances
por: Guillaume, C., et al.
Publicado: (2024)

How precisely can we measure the ages of subgiant and giant stars?
por: Shariat, Cheyanne, et al.
Publicado: (2025)

Quantifying the scale of star formation across the Perseus spiral arm using young clusters around Cas OB5
por: Quintana, Alexis L., et al.
Publicado: (2025)

Metallicity fluctuation statistics in the interstellar medium and young stars -- II. Elemental cross-correlations and the structure of chemical abundance space
por: Krumholz, Mark R., et al.
Publicado: (2025)

The internal kinematics of local young stellar associations. Identifying correlations among age, expansion, rotation, and shear
por: Olivares, J., et al.
Publicado: (2026)

The mass distribution of stars stripped in binaries: The effect of metallicity
por: Hovis-Afflerbach, B., et al.
Publicado: (2024)

Evolved stars with inconsistent age estimates: Abundance outliers or mass transfer products?
por: Frazer, Polly, et al.
Publicado: (2025)