Image de couverture de livre

Probing the wind and evolutionary state of the quiescent luminous blue variable Var$\,$2 in the Galaxy M33: constraints from self-consistent non-LTE modeling

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Kostenkov, A., Solovyeva, Y., Dedov, E., Vinokurov, A., Sarkisyan, A.
Format:	Preprint
Publié:	2025
Sujets:	Solar and Stellar Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

On the spatial distribution of luminous blue variables in the M33 galaxy
par: Kostenkov, A., et autres
Publié: (2025)

The Nature of the Emission Spectrum of NGC 7793 P13: modeling the atmosphere of the donor star
par: Vinokurov, A. S., et autres
Publié: (2024)

Simulations of massive star atmospheres and winds during giant eruptive and quiescent luminous blue variable phases
par: Schillemans, P., et autres
Publié: (2026)

The winds of OBA hypergiants and luminous blue variables: Dynamically-consistent atmosphere models reveal multiple wind regimes
par: Bernini-Peron, Matheus, et autres
Publié: (2026)

Modeling spectra of MN112
par: Kostenkov, A., et autres
Publié: (2020)

Search and Study of the Brightest Stars in the Galaxy IC 342
par: Sholukhova, O. N., et autres
Publié: (2024)

The solar beryllium abundance revisited with 3D non-LTE models
par: Amarsi, A. M., et autres
Publié: (2024)

Understanding an origin of palladium in metal-poor stars based on the non-LTE analysis of Pd~I lines
par: Mashonkina, L., et autres
Publié: (2025)

A statistical framework for quantitative spectroscopy of luminous blue stars
par: Urbaneja, Miguel A.
Publié: (2026)

The solar sulphur abundance in view of large-scale atomic structure calculations and 3D non-LTE models
par: Amarsi, A. M., et autres
Publié: (2025)

Photometric and spectroscopic variability of the blue supergiant rho Leo
par: Checha, V. A., et autres
Publié: (2025)

The IACOB project X. Large-scale quantitative spectroscopic analysis of Galactic luminous blue stars
par: de Burgos, Abel, et autres
Publié: (2023)

Evolution of rotating massive stars adopting a newer, self-consistent wind prescription at SMC metallicity
par: Gormaz-Matamala, Alex Camilo, et autres
Publié: (2024)

Prominence Plasma Parameters Maps Inferred From Lyman $β$ and Lyman $γ$ Observations and Non-LTE Modelling
par: Zhang, Y., et autres
Publié: (2026)

3D non-LTE abundance analyses of late-type stars
par: Lind, Karin, et autres
Publié: (2024)

Investigating non-LTE abundances of Neodymium (Nd) in metal-poor FGK stars
par: Dixon, John D., et autres
Publié: (2025)

Two successive EUV waves and a transverse oscillation of a quiescent prominence
par: Zhang, Q. M., et autres
Publié: (2024)

Non-evolutionary effects on period change in Magellanic Cepheids II. Empirical constraints on non-linear period changes
par: Rathour, Rajeev Singh, et autres
Publié: (2025)

Non-LTE abundances of nitrogen in the Sun and reference A-F type stars
par: Mashonkina, L. I., et autres
Publié: (2024)

A unified model of solar prominence formation with self-consistent heating
par: Huang, C. J., et autres
Publié: (2025)

Newly discovered Luminous blue variable candidates in M31 & M33
par: Li, Sai, et autres
Publié: (2026)

Influence of departures from LTE on determinations of the sulfur abundances in A-K type stars
par: Korotin, S. A., et autres
Publié: (2025)

Ag I model atom and the 3D non-LTE solar silver abundance
par: Caliskan, Sema, et autres
Publié: (2026)

New self-consistent theoretical descriptions for mass-loss rates of O-type stars
par: Figueroa-Tapia, F., et autres
Publié: (2026)

Further evidence of saturated, boosted, and disrupted magnetic braking from evolutionary tracks of cataclysmic variables
par: Barraza-Jorquera, Joaquín A., et autres
Publié: (2025)

Modeling of the magnetic stellar wind braking of the ssrAp 33 Lib (HD137949)
par: Nikiforov, A. G., et autres
Publié: (2026)

A distinct halo population revealed from 3D non-LTE magnesium abundances
par: Matsuno, T., et autres
Publié: (2024)

Role of non-thermal processes in the quiescent and active millimeter spectrum of a young M dwarf
par: Mohan, Atul, et autres
Publié: (2025)

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

Solar carbon abundance from 3D non-LTE modelling of the diagnostic lines of the CH molecule
par: Hoppe, Richard, et autres
Publié: (2025)

Non-LTE corrections for determinations of europium abundances in F-G-K stars in a broad metallicity range
par: Mashonkina, L. I., et autres
Publié: (2026)

Multiwavelength spectroscopic observations of a quiescent prominence
par: Xue, Jianchao, et autres
Publié: (2025)

The undetectable fraction of core-collapse supernovae in luminous infrared galaxies
par: Mäntynen, I., et autres
Publié: (2025)

Full non-LTE multi-level radiative transfer I. An atom with three bound infinitely sharp levels
par: Lagache, Tristan, et autres
Publié: (2025)

Towards a self-consistent hydrodynamical model of the solar tachocline
par: Garaud, P., et autres
Publié: (2025)

Examining the brightness variability, accretion disk, and evolutionary stage of the binary OGLE-LMC-ECL-14413
par: Mennickent, R. E., et autres
Publié: (2024)

Complex spectral variability and hints of a luminous companion in the Be star + black hole binary candidate ALS 8814
par: El-Badry, Kareem, et autres
Publié: (2025)

ALMAGAL II. The ALMA evolutionary study of high-mass protocluster formation in the Galaxy. ALMA data processing and pipeline
par: Sánchez-Monge, Á., et autres
Publié: (2025)

The evolutionary state of the red giant star L$_2$ Puppis
par: Uttenthaler, S.
Publié: (2024)

Three-dimensional non-LTE radiative transfer effects in Fe I lines IV. Line formation at high spatial resolution
par: Holzreuter, R., et autres
Publié: (2025)