Imagen de Portada

Neutron Star-Main Sequence Collisions Robustly Form Dynamically Stable Thorne-Żytkow Objects

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Williams, Lauryn E., Chang, Philip, Levesque, Emily M., Quinn, Thomas R.
Formato:	Preprint
Publicado:	2025
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

Thorne-Żytkow Objects
por: O'Grady, Anna J. G., et al.
Publicado: (2024)

Rethinking Thorne-Żytkow Object Formation: Assembly via Common Envelope in Field Binaries
por: Everson, Rosa Wallace, et al.
Publicado: (2023)

Population synthesis of Thorne-Żytkow objects: Rejuvenated donors and unexplored progenitors in the common envelope formation channel
por: Nathaniel, K., et al.
Publicado: (2024)

Unveiling Massive Main-Sequence Stars in Sextans A through Panchromatic Photometry
por: Gull, Maude, et al.
Publicado: (2026)

Rethinking Thorne-Żytkow Object Formation: The Fate of X-ray Binary LMC X-4 and Implications for Ultra-long Gamma-ray Bursts
por: Hutchinson-Smith, Tenley, et al.
Publicado: (2023)

Extended Main Sequences in Star Clusters
por: Li, Chengyuan, et al.
Publicado: (2024)

The Effect of Photometric Errors on the Measured Width of the Main Sequence in Star Clusters
por: Spangler, Steven R.
Publicado: (2025)

Broadening of the Main Sequence of a Star Cluster by Undetected Binaries
por: Spangler, Steven R.
Publicado: (2025)

The Status of the Astrophysical Parameters of Upper Main Sequence Stars
por: Kueß, Lukas, et al.
Publicado: (2025)

Chromospheric Mg I Emission Lines of Pre-Main-Sequence Stars
por: Yamashita, Mai, et al.
Publicado: (2024)

Why Do Stars Turn Red? I. Post-Main-Sequence Expansion Mechanism
por: Ou, Po-Sheng, et al.
Publicado: (2024)

Ultraviolet-Selected Field and Pre-Main-Sequence Stars Towards Taurus and Upper Scorpius
por: Findeisen, Krzysztof, et al.
Publicado: (2010)

Separating Photospheric and Starspot Magnetic Fields in Pre-Main-Sequence Stars Using IGRINS Spectroscopy
por: Paolino, Facundo Pérez, et al.
Publicado: (2025)

First Resolution of a Main Sequence G-Star Astrosphere Using Chandra
por: Lisse, C. M., et al.
Publicado: (2025)

Modelling the Future of Gaia Neutron Star-Main Sequence Binaries: From Eccentric Orbits to Millisecond Pulsar-White Dwarfs
por: Chattopadhyay, Debatri, et al.
Publicado: (2025)

Five New Sirius-Like White Dwarf + Main Sequence Star Systems with MagAO-X
por: Pearce, Logan A., et al.
Publicado: (2025)

Dynamical Masses for 23 Pre-Main Sequence Stars in Upper Scorpius: A Critical Test of Stellar Evolutionary Models
por: Towner, A. P. M., et al.
Publicado: (2025)

Surprisingly Similar: The Mass Function of Gaia Neutron Stars and First-Born Double Neutron Stars
por: Schiebelbein-Zwack, Aryanna, et al.
Publicado: (2025)

Characterizing the Low-Mass Pre-Main-Sequence Population in the Low-Metallicity Star-Forming Region Dolidze 25 Using VLT-MUSE
por: Ashraf, Mizna, et al.
Publicado: (2025)

Older Ages for 23 Pre-Main Sequence Stars in Upper Scorpius Using Dynamical Mass-Constrained Stellar Evolutionary Models
por: Towner, Allison P. M., et al.
Publicado: (2026)

Neutron Star Atmosphere-Ocean Dynamics
por: Nättilä, Joonas, et al.
Publicado: (2023)

Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus
por: Yang, Mingkuan, et al.
Publicado: (2026)

Rotating Supermassive Pop III Stars On The Main Sequence
por: Nandal, Devesh, et al.
Publicado: (2025)

The California Legacy Survey V. Chromospheric Activity Cycles in Main Sequence Stars
por: Isaacson, Howard, et al.
Publicado: (2024)

A Systematic Search for Main-Sequence Dipper Stars Using the Zwicky Transient Facility
por: Tzanidakis, Anastasios, et al.
Publicado: (2025)

Lithium Abundances of Main-Sequence Stars in the Old Open Cluster NGC 188: Probes of Stellar Evolution Beyond the Solar Age
por: Sun, Qinghui, et al.
Publicado: (2025)

Stars of the Lower Part of the Main Sequence with Discovered Exoplanets and Candidates. Periods of Rotations or Revolutions?
por: Shlyapnikov, Aleksey A.
Publicado: (2024)

Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers
por: Qin, Ying, et al.
Publicado: (2024)

Habitable Zones Around Massive Stars: From the Main Sequence to Supergiants
por: Nandal, Devesh, et al.
Publicado: (2026)

Untangling the Sources of Abundance Dispersion in Low-metallicity Stars II: Neutron Capture Elements
por: Griffith, Emily J., et al.
Publicado: (2025)

The Dynamic Inner Disk of a Planet Forming Star
por: Setterholm, Benjamin R., et al.
Publicado: (2025)

Millions of Main-Sequence Binary Stars from Gaia BP/RP Spectra
por: Li, Jiadong, et al.
Publicado: (2025)

The Cohesive Object Sequence: The Mass-Density Distribution of Astronomical Objects from Asteroids to Stars
por: Steward, Gabriel M, et al.
Publicado: (2026)

Asteroseismology and Dynamics Reveal Interior Structure and Coeval Evolution in the Triply Post-Main-Sequence system DG Leo
por: Li, Ping, et al.
Publicado: (2025)

Haro 5-2: A New Pre-Main Sequence Quadruple Stellar System
por: Reipurth, Bo, et al.
Publicado: (2024)

Fast Pulsars, Neutron Stars, and Astrophysical Strange Quark Matter Objects
por: Farrell, Delaney, et al.
Publicado: (2024)

Growth of Metal-Enriched Supermassive Stars by Accretion and Collisions
por: Nandal, Devesh, et al.
Publicado: (2025)

SZ Lyncis: A Non-Accreting Neutron Star-delta Scuti Binary Candidate Discovered via Dynamics and Asteroseismology
por: Li, Ping, et al.
Publicado: (2024)

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)

In Search of Decay: An Analysis of Transit Times of Hot Jupiters in Main Sequence and Post-Main Sequence Systems
por: Sodickson, Noah, et al.
Publicado: (2025)