Imagen de Portada

Elusive hot stripped helium stars in the Galaxy I. Evolutionary stellar models in the gap between subdwarfs and Wolf-Rayet stars

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Yungelson, L., Kuranov, A., Postnov, K., Kuranova, M., Oskinova, L., Hamann, W. -R.
Formato:	Preprint
Publicado:	2024
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

Elusive helium stars in the gap between subdwarfs and Wolf-Rayet stars~II. Nonlinear pulsations of stripped helium stars
por: Fadeyev, Yu. A., et al.
Publicado: (2025)

A comprehensive search for hot subdwarf stars using Gaia and TESS I. Pulsating hot subdwarf B stars
por: Uzundag, Murat, et al.
Publicado: (2024)

Near-Eddington mass loss of hydrogen-rich Wolf-Rayet stars
por: Lefever, Roel R., et al.
Publicado: (2025)

The population synthesis of Wolf-Rayet stars involving binary merger channels
por: Li, Zhuowen, et al.
Publicado: (2024)

The $i$-processes nucleosynthesis during the formation of He-rich hot-subdwarf stars
por: Battich, T., et al.
Publicado: (2025)

The SALT survey of helium-rich hot subdwarfs: unsupervised classification and kinematic analysis
por: Monai, Asish Philip, et al.
Publicado: (2026)

The enigmatic winds of Wolf-Rayet stars: Results from dynamically consistent atmosphere modelling
por: Sander, Andreas A. C.
Publicado: (2022)

Impact of main-sequence mass loss on the appearance, structure and evolution of Wolf-Rayet stars
por: Josiek, Joris, et al.
Publicado: (2024)

Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars II. Sample validation
por: Benitez-Palacios, Diego, et al.
Publicado: (2025)

Can Wolf-Rayet stars be the missing ingredient to explain high-z He II ionizing radiation?
por: González-Torà, G., et al.
Publicado: (2025)

New empirical mass-loss recipe for UV radiation line-driven winds of hot stars across various metallicities
por: Pauli, D., et al.
Publicado: (2025)

Determining stellar properties of massive stars in NGC346 in the SMC with a Bayesian statistic technique
por: Rickard, M. J., et al.
Publicado: (2024)

Search for new Galactic Wolf-Rayet stars using Gaia DR3. I. Candidate selection and the follow-up of the bright sample
por: Mulato, Lionel, et al.
Publicado: (2025)

On the Spatial Distribution of Luminous Blue Variables, B[e] Supergiants, and Wolf-Rayet stars in the Large Magellanic Cloud
por: Martin, John C., et al.
Publicado: (2025)

Ring nebulae around Wolf-Rayet stars in M33 as seen by SITELLE
por: Tuquet, Selin, et al.
Publicado: (2024)

Classification of Wolf Rayet stars using Ensemble-based Machine Learning algorithms
por: Kar, Subhajit, et al.
Publicado: (2024)

On the evolutionary nature of puffed-up stripped star binaries and their occurrence in stellar populations
por: Dutta, Debasish, et al.
Publicado: (2023)

Detection of hot subdwarf binaries and sdB stars using machine learning methods and a large sample of Gaia XP spectra
por: Ambrosch, M., et al.
Publicado: (2026)

The Discovery of Three Galactic Wolf-Rayet Stars
por: Marin, Laurella C., et al.
Publicado: (2024)

Evolutionary Map of the Universe: Detection and Analysis of the Shell Surrounding the Runaway Wolf-Rayet Star WR16
por: Bradley, A. C., et al.
Publicado: (2025)

A spectroscopic and kinematic survey of fast hot subdwarfs
por: Geier, S., et al.
Publicado: (2024)

An absence of binary companions to Wolf-Rayet stars in the Small Magellanic Cloud: implications for mass loss and black hole masses at low metallicity
por: Schootemeijer, A., et al.
Publicado: (2024)

X-ray and radio data obtained by XMM-Newton and VLA constrain the stellar wind of the magnetic quasi-Wolf-Rayet star in HD45166
por: Leto, P., et al.
Publicado: (2025)

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

Empirical correlation between masses of black holes and Wolf-Rayet stars derived from their mass distributions in spectroscopic binaries
por: Postnov, Konstantin, 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)

Extremely iron-poor O-type stars in the Magellanic Bridge
por: Schösser, E. C., et al.
Publicado: (2025)

Investigating 39 Galactic Wolf-Rayet stars with VLTI/GRAVITY: Uncovering A Long Period Binary Desert
por: Deshmukh, K., et al.
Publicado: (2024)

Formation and Evolution of [Wolf-Rayet] Planetary Nebulae through a Late Thermal Pulse
por: Rodríguez-González, J. B., et al.
Publicado: (2026)

Outflow from the very massive Wolf-Rayet binary Melnick 34
por: Castro, N., et al.
Publicado: (2024)

The Nature of a Recently Discovered Wolf-Rayet Binary: Archetype of Stripping?
por: Massey, Philip, et al.
Publicado: (2024)

Wolf-Rayet stars
por: Shenar, Tomer
Publicado: (2024)

Massive stellar cannibals: How stellar mergers drive mass-loss in extremely massive stars
por: Roman-Garza, J., et al.
Publicado: (2026)

The Aromatic Infrared Bands around the Wolf-Rayet Binary WR140 Revealed by JWST
por: Taniguchi, Kotomi, et al.
Publicado: (2025)

Lightcurves of stars in the Chamaeleon I Association
por: Neumannová, K., et al.
Publicado: (2025)

Structure formation in O-type stars and Wolf-Rayet stars
por: Van der Sijpt, C., et al.
Publicado: (2025)

X-Shooting ULLYSES: Massive stars at low metallicity. III. Terminal wind speeds of ULLYSES massive stars
por: Hawcroft, C., et al.
Publicado: (2023)

Parametric models of core-helium-burning stars: structural glitches near the core
por: Matteuzzi, Massimiliano, et al.
Publicado: (2025)

X-Shooting ULLYSES: Massive Stars at low metallicity VIII. Stellar and wind parameters of newly revealed stripped stars in Be binaries
por: Ramachandran, V., et al.
Publicado: (2024)

Primeval very low-mass stars and brown dwarfs -- VIII. The first age benchmark L subdwarf, a wide companion to a halo white dwarf
por: Zhang, Z. H., et al.
Publicado: (2024)