Stellar Physics Across the HR Diagram with Gaia
Fuente:
arXiv
Guardado en:
| Autor principal: | Creevey, Orlagh L. |
|---|---|
| Formato: | Preprint |
| Publicado: |
2025
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Exploring Young Stellar Variability with Gaia DR3 light curves
por: Mas, Chloé, et al.
Publicado: (2025)
por: Mas, Chloé, et al.
Publicado: (2025)
Exoplanets Across Galactic Stellar Populations with PLATO: Estimating Exoplanet Yields Around FGK Stars for the Thin Disk, Thick Disk and Stellar Halo
por: Boettner, Christopher, et al.
Publicado: (2024)
por: Boettner, Christopher, et al.
Publicado: (2024)
The Gaia Ultracool Dwarf Sample -- IV. GTC/OSIRIS optical spectra of Gaia late-M and L dwarfs
por: Cooper, W. J., et al.
Publicado: (2024)
por: Cooper, W. J., et al.
Publicado: (2024)
The Gaia white dwarf revolution
por: Tremblay, Pier-Emmanuel, et al.
Publicado: (2024)
por: Tremblay, Pier-Emmanuel, et al.
Publicado: (2024)
A Census of the beta Pic Moving Group and Other Nearby Associations with Gaia
por: Luhman, K. L.
Publicado: (2024)
por: Luhman, K. L.
Publicado: (2024)
Gaia search for stellar companions of TESS Objects of Interest V
por: Mugrauer, M., et al.
Publicado: (2025)
por: Mugrauer, M., et al.
Publicado: (2025)
Stellar Flares Are Far-Ultraviolet Luminous
por: Berger, Vera L., et al.
Publicado: (2023)
por: Berger, Vera L., et al.
Publicado: (2023)
The Gaia Ultracool Dwarf Sample -- V: The Ultracool Dwarf Companion catalogue
por: Baig, Sayan, et al.
Publicado: (2024)
por: Baig, Sayan, et al.
Publicado: (2024)
Resolving the Super-Earth/Gas Giant Connection in Stellar Mass and Metallicity
por: Bryan, Marta L., et al.
Publicado: (2025)
por: Bryan, Marta L., et al.
Publicado: (2025)
Eccentricities of Close Stellar Binaries
por: Wu, Yanqin, et al.
Publicado: (2024)
por: Wu, Yanqin, et al.
Publicado: (2024)
Near-infrared spectroscopic characterisation of Gaia ultra-cool dwarf candidates; Spectral types and peculiarities
por: Ravinet, T., et al.
Publicado: (2024)
por: Ravinet, T., et al.
Publicado: (2024)
Star formation and accretion rates within 500 pc as traced by Gaia DR3 XP spectra
por: Delfini, L., et al.
Publicado: (2025)
por: Delfini, L., et al.
Publicado: (2025)
The Gaia Ultracool Dwarf Sample -- VI. Spectral Types and Properties of 51 Ultracool Dwarfs
por: Cheng, Gemma, et al.
Publicado: (2025)
por: Cheng, Gemma, et al.
Publicado: (2025)
A close binary lens revealed by the microlensing event Gaia20bof
por: Bachelet, E., et al.
Publicado: (2024)
por: Bachelet, E., et al.
Publicado: (2024)
Microlensing Constraints on the Stellar and Planetary Mass Functions
por: Yee, Jennifer C., et al.
Publicado: (2025)
por: Yee, Jennifer C., et al.
Publicado: (2025)
Identifying Hierarchically Triple Star Systems with Gaia DR3 and LAMOST
por: He, Tongyu, et al.
Publicado: (2024)
por: He, Tongyu, et al.
Publicado: (2024)
Validation of Gaia DR3 orbital and acceleration solutions with hierarchical triples
por: Nagarajan, Pranav, et al.
Publicado: (2024)
por: Nagarajan, Pranav, et al.
Publicado: (2024)
Stability of a cluster-disrupted mean-motion resonance (chain) in HR 8799 and PDS 70
por: Maas, Brent, et al.
Publicado: (2025)
por: Maas, Brent, et al.
Publicado: (2025)
Lost Sisters Found: TESS and Gaia Reveal a Dissolving Pleiades Complex
por: Boyle, Andrew W., et al.
Publicado: (2025)
por: Boyle, Andrew W., et al.
Publicado: (2025)
Kepler meets Gaia DR3: homogeneous extinction-corrected color-magnitude diagram and binary classification
por: Godoy-Rivera, D., et al.
Publicado: (2025)
por: Godoy-Rivera, D., et al.
Publicado: (2025)
A Kinematic History of Stellar Encounters with Beta Pictoris
por: Gragera-Más, Jose Luis, et al.
Publicado: (2025)
por: Gragera-Más, Jose Luis, et al.
Publicado: (2025)
Stellar companions and Jupiter-like planets in young associations
por: Gratton, R., et al.
Publicado: (2024)
por: Gratton, R., et al.
Publicado: (2024)
A Data-driven Spectral Model of Main Sequence Stars in Gaia DR3
por: Angelo, Isabel, et al.
Publicado: (2024)
por: Angelo, Isabel, et al.
Publicado: (2024)
Correlations between Ca II H&K Emission and the Gaia M dwarf Gap
por: Boudreaux, Emily M., et al.
Publicado: (2024)
por: Boudreaux, Emily M., et al.
Publicado: (2024)
Search for Past Stellar Encounters and the Origin of 3I/ATLAS
por: Guo, Yiyang, et al.
Publicado: (2025)
por: Guo, Yiyang, et al.
Publicado: (2025)
Stellar encounters in the solar neighbourhood and the special case of GJ~710
por: Fernandez-Puig, Eloi, et al.
Publicado: (2026)
por: Fernandez-Puig, Eloi, et al.
Publicado: (2026)
The GRAVITY Young Stellar Object survey. VII. The inner dusty disks of T Tauri stars
por: The GRAVITY Collaboration, et al.
Publicado: (2021)
por: The GRAVITY Collaboration, et al.
Publicado: (2021)
SED Modeling of Young Stellar Objects in the Orion Star Formation Complex
por: Gezer, Ilknur, et al.
Publicado: (2025)
por: Gezer, Ilknur, et al.
Publicado: (2025)
Dynamical Architectures of S-type Transiting Planets in Binaries I: Target Selection using Hipparcos and Gaia proper motion anomalies
por: Zhang, Jingwen, et al.
Publicado: (2023)
por: Zhang, Jingwen, et al.
Publicado: (2023)
Photometric Stellar Parameters for 195,478 Kepler Input Catalog (KIC) Stars
por: Zhang, Bowen, et al.
Publicado: (2024)
por: Zhang, Bowen, et al.
Publicado: (2024)
Thermal Structure Determines Kinematics: Vertical Shear Instability in Stellar Irradiated Protoplanetary Disks
por: Zhang, Shangjia, et al.
Publicado: (2024)
por: Zhang, Shangjia, et al.
Publicado: (2024)
paired: A Statistical Framework for Detecting Stellar Binarity with Gaia RVs. I. Sensitivity to Unresolved Binaries
por: Chance, Quadry, et al.
Publicado: (2022)
por: Chance, Quadry, et al.
Publicado: (2022)
Stellar flybies within 1 ly from the Sun and stars passing through the Hills cloud
por: Potemine, Igor Yu.
Publicado: (2024)
por: Potemine, Igor Yu.
Publicado: (2024)
Orbits and Masses for 156 Companions from Combined Astrometry and Radial Velocities, and A Validation of Gaia Non-Single Star Solutions
por: An, Qier, et al.
Publicado: (2025)
por: An, Qier, et al.
Publicado: (2025)
Solar Periodic Companion and Random Stellar Flybys: Dynamical Perturbations of Highly Eccentric Comets in the Oort Cloud
por: Arani, Shahed Shayan
Publicado: (2025)
por: Arani, Shahed Shayan
Publicado: (2025)
Improving Accretion Diagnostics for Young Stellar Objects with Mid-infrared Hydrogen lines from JWST/MIRI
por: Shridharan, B, et al.
Publicado: (2025)
por: Shridharan, B, et al.
Publicado: (2025)
Stellar Characterization and a Chromospheric Activity Analysis of a K2 Sample of Planet-Hosting Stars
por: Loaiza-Tacuri, V., et al.
Publicado: (2024)
por: Loaiza-Tacuri, V., et al.
Publicado: (2024)
Distributions of wide binary stars in theory and in Gaia data: I. Generalized Ambartsumian (1937) approach and the family of power-law distributions of eccentricity
por: Makarov, Valeri V.
Publicado: (2025)
por: Makarov, Valeri V.
Publicado: (2025)
The Radiowave Hunt for Young Stellar Object Emission and Demographics (RADIOHEAD): A Radio Luminosity${-}$Spectral Type Dependence in Taurus${-}$Auriga YSOs
por: Rahman, Ramisa Akther, et al.
Publicado: (2025)
por: Rahman, Ramisa Akther, et al.
Publicado: (2025)
Disentangling Metallicity Effects in Hot Jupiter Occurrence Across Galactic Birth Radius and Phase-Space Density
por: Rampalli, Rayna, et al.
Publicado: (2025)
por: Rampalli, Rayna, et al.
Publicado: (2025)
Ejemplares similares
-
Exploring Young Stellar Variability with Gaia DR3 light curves
por: Mas, Chloé, et al.
Publicado: (2025) -
Exoplanets Across Galactic Stellar Populations with PLATO: Estimating Exoplanet Yields Around FGK Stars for the Thin Disk, Thick Disk and Stellar Halo
por: Boettner, Christopher, et al.
Publicado: (2024) -
The Gaia Ultracool Dwarf Sample -- IV. GTC/OSIRIS optical spectra of Gaia late-M and L dwarfs
por: Cooper, W. J., et al.
Publicado: (2024) -
The Gaia white dwarf revolution
por: Tremblay, Pier-Emmanuel, et al.
Publicado: (2024) -
A Census of the beta Pic Moving Group and Other Nearby Associations with Gaia
por: Luhman, K. L.
Publicado: (2024)