Imagen de Portada

A Multi-Method Age Determination for the Ursa Major Moving Group

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Sheffler, Julia, Clark, Max, Soares-Furtado, Melinda, Distler, Adam, Narayan, Ritvik Sai, Karcheski, Jenna, Nordsieck, Kenneth
Formato:	Preprint
Publicado:	2026
Materias:	Solar and Stellar Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

The Tale of a Hungry Subgiant and Its Brown Dwarf: Interior Radiative Damping Dominates the Tidal Evolution of TOI-5882
por: Narayan, Ritvik Sai, et al.
Publicado: (2026)

TESS Hunt for Young and Maturing Exoplanets (THYME) XIV: A Comoving-Based Age Constraint for KELT-20
por: Distler, Adam, et al.
Publicado: (2026)

Twinkle Twinkle Little Star, Roman Sees Where You Are: Predicting Exoplanet Transit Yields in the Rosette Nebula with the Nancy Grace Roman Space Telescope
por: Narayan, Ritvik Sai, et al.
Publicado: (2025)

TESS Hunt for Young and Maturing Exoplanets (THYME) XI: An Earth-sized Planet Orbiting a Nearby, Solar-like Host in the 400Myr Ursa Major Moving Group
por: Capistrant, Benjamin K., et al.
Publicado: (2024)

Give to Ursa Minor what is Ursa Minor's: an updated census of the RR Lyrae population in the Ursa Minor dwarf galaxy based on Gaia DR3
por: Garofalo, A., et al.
Publicado: (2024)

WIYN Open Cluster Study. XCVII. An Extended Radial-Velocity Survey and Spectroscopic Binary Orbits in the Open Cluster NGC 188
por: Narayan, Ritvik Sai, et al.
Publicado: (2025)

Host Stars and How Their Compositions Influence Exoplanets
por: Hinkel, Natalie R., et al.
Publicado: (2024)

Chemical enrichment of metal-poor stars orbiting massive black hole companions
por: Rosselli-Calderon, Alejandra, et al.
Publicado: (2025)

The Binary Fraction of Stars in the Dwarf Galaxy Ursa Minor via Dark Energy Spectroscopic Instrument
por: Qiu, Tian, et al.
Publicado: (2025)

Flare frequency in M dwarfs belonging to Young Moving Groups
por: Mamonova, E., et al.
Publicado: (2025)

Observable Metal Pollution in Main-Sequence Stars: Simulations of Rocky Planets Engulfed by Stars in the $0.5$ to $1.4$ M$_\odot$ Range
por: Lane, Kaitlyn T., et al.
Publicado: (2026)

Reassessing the Relationship Between Stellar X-ray Luminosity and Age with eROSITA Data Release 1
por: Quiñones, Nadja Aldarondo, et al.
Publicado: (2025)

Spectroscopic Characterization of WD J000801.25-350450 and its Two Co-Moving Companions
por: Jałowiczor, Peter A., et al.
Publicado: (2026)

Flaring Activity for Low-Mass Stars in the $β$ Pictoris Moving Group
por: Ealy, Jordan N., et al.
Publicado: (2024)

What's Their Age Again? A Blue-Straggler Merger Scenario in the $γ$ Persei Binary System
por: Tarczay-Nehéz, D., et al.
Publicado: (2026)

The Decay of Two Adjacent Sunspots Associated with Moving Magnetic Features
por: Peng, Yang, et al.
Publicado: (2024)

Chemistry and Isotope Ratios of Substellar Atmospheres in the $β$ Pictoris Young Moving Group
por: Liu, Yurou, et al.
Publicado: (2026)

Automated Methods for Abundance Determination
por: Prieto, Carlos Allende
Publicado: (2025)

Solar Orbiter's 2024 Major Flare Campaigns: An Overview
por: Ryan, Daniel F., et al.
Publicado: (2025)

Moving Plasma Structures and Possible Driving Mechanisms of Solar Microflares Observed with High-Resolution Coronal Imaging
por: Wang, Qingmei, et al.
Publicado: (2025)

Binary Systems Search with TESS
por: Otani, Tomomi, et al.
Publicado: (2025)

New Approach to Superflare Energy Determination
por: Heinzel, Petr, et al.
Publicado: (2026)

The Stationary Point: A New Method for Solar Wind Speed Measurements from a Moving Vantage Point
por: Van Kooten, Samuel J., et al.
Publicado: (2025)

The Silent Majority: The Interacting Post-Common-Envelope Binaries Underlying Cataclysmic Variables
por: Shani, Yarin Meir, et al.
Publicado: (2025)

Unveiling stellar spin: Determining inclination angles in Be stars
por: Turis-Gallo, D., et al.
Publicado: (2025)

Microwave Imaging Spectroscopy Diagnosis of the Slow-rise Precursor of a Major Solar Eruption
por: Kou, Yuankun, et al.
Publicado: (2025)

A Major Geomagnetic Storm in 2024 October Linked to Sympathetic CME--Prominence Eruptions
por: Wang, Rui, et al.
Publicado: (2026)

The Andromeda Galaxy's Last Major Merger: Constraints from the survey of Planetary Nebulae
por: Bhattacharya, Souradeep, et al.
Publicado: (2023)

Determining the magnetic field of active region plages using the whole CLASP2/2.1 spectral window
por: Delgado, David Afonso, et al.
Publicado: (2025)

Determination of the Solar System contribution to the soft X-ray sky
por: Dennerl, K., et al.
Publicado: (2026)

Determining the Magnetic Field in the Atmosphere of a Solar Active Region Observed by the CLASP2.1 Sounding Rocket Experiment
por: Ishikawa, Ryohko, et al.
Publicado: (2025)

Age Determination of LAMOST Red Giant Branch stars based on the Gradient Boosting Decision Tree method
por: Wang, Hai-Feng, et al.
Publicado: (2023)

Relationship Between Major Stellar Physical Parameters and Normal Mode Frequencies in Accreting White Dwarf Stars
por: Kumar, Praphull, et al.
Publicado: (2025)

The Birth of a Major Coronal Mass Ejection with Intricate Magnetic Structure from Multiple Active Regions
por: Guo, Jinhan, et al.
Publicado: (2025)

Determining the incidence rate of magnetic $δ$ Scuti candidates with CoRoT
por: Paul, Gautam, et al.
Publicado: (2026)

Turbulence inference from CO spectral observations
por: Narayan, Jayashree, et al.
Publicado: (2025)

New insight into the variability of the Be star $π$ Aquarii: Determination of stellar and disk parameters
por: Concha, D., et al.
Publicado: (2025)

Emission Measures Demystified
por: Dennis, Brian R., et al.
Publicado: (2024)

Nested active regions anchor the heliospheric current sheet and stall the reversal of the coronal magnetic field
por: Finley, Adam J.
Publicado: (2024)

Stellar flares
por: Kowalski, Adam F.
Publicado: (2024)