Saved in:
| Main Authors: | Nathaniel, K., Langer, N., Simón-Díaz, S., Holgado, G., de Burgos, A., Hastings, B. |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | https://arxiv.org/abs/2502.12107 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
The IACOB project XIV. New clues on the location of the TAMS in the massive star domain
by: de Burgos, A., et al.
Published: (2025)
by: de Burgos, A., et al.
Published: (2025)
Magnetic field generation in mergers of massive main sequence stars
by: Ohlmann, Sebastian T., et al.
Published: (2025)
by: Ohlmann, Sebastian T., et al.
Published: (2025)
The IACOB project: CVIII. Hunting for spectroscopic binaries in the O and B supergiant domain.The threat of pulsational variability
by: Simón-Díaz, S., et al.
Published: (2024)
by: Simón-Díaz, S., et al.
Published: (2024)
The IACOB project XV. Updated calibrations of fundamental parameters of Galactic O-type stars
by: Holgado, G., et al.
Published: (2025)
by: Holgado, G., et al.
Published: (2025)
The IACOB project XIII. Helium enrichment in O-type stars as a tracer of past binary interaction
by: Martínez-Sebastián, C., et al.
Published: (2024)
by: Martínez-Sebastián, C., et al.
Published: (2024)
Multiplicity of Massive stars in the Milky Way (M3W). I. Project description, UNWIND, application to GLS 11 448, and DIB catalog
by: Apellániz, J. Maíz, et al.
Published: (2026)
by: Apellániz, J. Maíz, et al.
Published: (2026)
A magnetic field detection in the massive O-type bright giant 63 Oph
by: Barron, James A., et al.
Published: (2025)
by: Barron, James A., et al.
Published: (2025)
3D hydrodynamic simulations of massive main-sequence stars -- IV. Internal gravity waves matter for SLF variability
by: Pathak, Praneet, et al.
Published: (2025)
by: Pathak, Praneet, et al.
Published: (2025)
Open questions in massive star research
by: Langer, N.
Published: (2022)
by: Langer, N.
Published: (2022)
Chemically peculiar stars on the pre-main sequence
by: Kueß, L., et al.
Published: (2024)
by: Kueß, L., et al.
Published: (2024)
Pre-main sequence stars
by: Semkov, Evgeni
Published: (2023)
by: Semkov, Evgeni
Published: (2023)
Asteroseismic predictions for a massive main-sequence merger product
by: Henneco, J., et al.
Published: (2025)
by: Henneco, J., et al.
Published: (2025)
3D hydrodynamic simulations of massive main-sequence stars II. Convective excitation and spectra of internal gravity waves
by: Thompson, William, et al.
Published: (2023)
by: Thompson, William, et al.
Published: (2023)
Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
by: Jin, Harim, et al.
Published: (2024)
by: Jin, Harim, et al.
Published: (2024)
The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars
by: Martínez-Sebastián, C., et al.
Published: (2026)
by: Martínez-Sebastián, C., et al.
Published: (2026)
Variations in the magnetic field strength of pre-main-sequence stars, solar-type main-sequence stars, and the Sun
by: Yamashita, Mai, et al.
Published: (2025)
by: Yamashita, Mai, et al.
Published: (2025)
The impact of disk-locking on convective turnover times of low-mass pre-main sequence and main sequence stars
by: Landin, N. R., et al.
Published: (2024)
by: Landin, N. R., et al.
Published: (2024)
How large spectroscopic surveys are shaping our understanding of massive stars
by: Simón-Díaz, S.
Published: (2026)
by: Simón-Díaz, S.
Published: (2026)
On the response of massive main sequence stars to mass accretion and outflow at high rates
by: Bear, Ealeal, et al.
Published: (2024)
by: Bear, Ealeal, et al.
Published: (2024)
Obscured star clusters in the Inner Milky Way. How many massive young clusters are still awaiting detection?
by: Gupta, Akash, et al.
Published: (2024)
by: Gupta, Akash, et al.
Published: (2024)
The accretion history of the Milky Way IV. Hints of recent star formation in Milky Way dwarf spheroidal galaxies
by: Yang, Yanbin, et al.
Published: (2024)
by: Yang, Yanbin, et al.
Published: (2024)
3D hydrodynamic simulations of massive main-sequence stars. III. The effect of radiation pressure and diffusion leading to a 1D equilibrium model
by: Mao, Huaqing, et al.
Published: (2023)
by: Mao, Huaqing, et al.
Published: (2023)
Kepler main-sequence solar-like stars: surface rotation and magnetic-activity evolution
by: Santos, A. R. G., et al.
Published: (2024)
by: Santos, A. R. G., et al.
Published: (2024)
Pulsation in hot main sequence stars: comparison of observations with models
by: Balona, Luis A.
Published: (2023)
by: Balona, Luis A.
Published: (2023)
Chemical tracers of a highly eccentric AGB-main sequence star binary
by: Danilovich, T., et al.
Published: (2024)
by: Danilovich, T., et al.
Published: (2024)
The IACOB project: XVI. Surface helium abundances in Galactic O-type stars: indications for identifying binary interaction products
by: Simón-Díaz, S., et al.
Published: (2026)
by: Simón-Díaz, S., et al.
Published: (2026)
The Mass Dependence of Hα Emission and Stellar Spindown for Fully Convective M Dwarfs
by: Pass, Emily K., et al.
Published: (2024)
by: Pass, Emily K., et al.
Published: (2024)
X-ray detection of astrospheres around three main-sequence stars and their mass-loss rates
by: Kislyakova, K. G., et al.
Published: (2024)
by: Kislyakova, K. G., et al.
Published: (2024)
Evolution of stars with 60 and 200 Msun: predictions for WNh stars in the Milky Way
by: Gormaz-Matamala, Alex Camilo, et al.
Published: (2024)
by: Gormaz-Matamala, Alex Camilo, et al.
Published: (2024)
Analysis of mass-transferring binary candidates in the Milky Way
by: Garcia-Moreno, G., et al.
Published: (2025)
by: Garcia-Moreno, G., et al.
Published: (2025)
Externally irradiated young stars in NGC 3603. A JWST NIRSpec catalogue of pre-main-sequence stars in a massive star formation region
by: Rogers, Ciarán, et al.
Published: (2024)
by: Rogers, Ciarán, et al.
Published: (2024)
Investigating episodic mass loss in evolved massive stars: III. Spectroscopy of dusty massive stars in three northern galaxies
by: de Wit, S., et al.
Published: (2025)
by: de Wit, S., et al.
Published: (2025)
Axisymmetric second order perturbations of rotating main sequence stars
by: Lee, Umin
Published: (2025)
by: Lee, Umin
Published: (2025)
Observational signs of limited flare area variation and peak flare temperatures estimations in main-sequence flaring stars
by: Bicz, K., et al.
Published: (2025)
by: Bicz, K., et al.
Published: (2025)
Debris disks around main-sequence stars
by: Pearce, Tim D.
Published: (2024)
by: Pearce, Tim D.
Published: (2024)
NGC 663 as a laboratory for massive star evolution
by: Marco, Amparo, et al.
Published: (2025)
by: Marco, Amparo, et al.
Published: (2025)
Magnetic Fields in the Bones of the Milky Way
by: Stephens, Ian W., et al.
Published: (2025)
by: Stephens, Ian W., et al.
Published: (2025)
Radial differential rotation leading to dipole collapse in pre-main-sequence stars
by: Guseva, A., et al.
Published: (2026)
by: Guseva, A., et al.
Published: (2026)
How many stars form in compact clusters in the local Milky Way?
by: Quintana, Alexis L., et al.
Published: (2025)
by: Quintana, Alexis L., et al.
Published: (2025)
How Gaia sheds light on the Milky Way star cluster population
by: Cantat-Gaudin, T., et al.
Published: (2024)
by: Cantat-Gaudin, T., et al.
Published: (2024)
Similar Items
-
The IACOB project XIV. New clues on the location of the TAMS in the massive star domain
by: de Burgos, A., et al.
Published: (2025) -
Magnetic field generation in mergers of massive main sequence stars
by: Ohlmann, Sebastian T., et al.
Published: (2025) -
The IACOB project: CVIII. Hunting for spectroscopic binaries in the O and B supergiant domain.The threat of pulsational variability
by: Simón-Díaz, S., et al.
Published: (2024) -
The IACOB project XV. Updated calibrations of fundamental parameters of Galactic O-type stars
by: Holgado, G., et al.
Published: (2025) -
The IACOB project XIII. Helium enrichment in O-type stars as a tracer of past binary interaction
by: Martínez-Sebastián, C., et al.
Published: (2024)