Rapid polarization variations in the O4 supergiant $ζ$ Puppis
Fuente:
arXiv
Guardado en:
| Autores principales: | Bailey, Jeremy, Howarth, Ian D., Cotton, Daniel V., Kedziora-Chudczer, Lucyna, De Horta, Ain, Martell, Sarah L., Eldridge, Colin, Luckas, Paul |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Epsilon Sagittarii: An Extreme Rapid Rotator with a Decretion Disk
por: Bailey, Jeremy, et al.
Publicado: (2024)
por: Bailey, Jeremy, et al.
Publicado: (2024)
Polarization position angle standard stars: a reassessment of $θ$ and its variability for seventeen stars based on a decade of observations
por: Cotton, Daniel V., et al.
Publicado: (2024)
por: Cotton, Daniel V., et al.
Publicado: (2024)
Spectro Capture: A Software System for Automated Small-Observatory Spectroscopy
por: Luckas, Paul
Publicado: (2026)
por: Luckas, Paul
Publicado: (2026)
Observed epochal variations in X-ray lines from the O Supergiant $ζ$ Puppis do not require substantial changes in the wind mass flux
por: Gunderson, Sean J., et al.
Publicado: (2024)
por: Gunderson, Sean J., et al.
Publicado: (2024)
Absolute Parameters of Young Stars: NO Puppis
por: Erdem, Ahmet, et al.
Publicado: (2025)
por: Erdem, Ahmet, et al.
Publicado: (2025)
Deneb is a Large Amplitude Polarimetric Variable
por: Cotton, Daniel V., et al.
Publicado: (2024)
por: Cotton, Daniel V., et al.
Publicado: (2024)
Detection of dark companions via the combination of eclipse timing variation, Hipparcos and/or Gaia astrometry: the cases of V Puppis and CY Ari
por: Xiao, Guang-Yao, et al.
Publicado: (2025)
por: Xiao, Guang-Yao, et al.
Publicado: (2025)
The evolutionary state of the red giant star L$_2$ Puppis
por: Uttenthaler, S.
Publicado: (2024)
por: Uttenthaler, S.
Publicado: (2024)
Interferometric Images of the Starspot Evolution of $ζ$ Andromedae
por: Roettenbacher, Rachael M., et al.
Publicado: (2026)
por: Roettenbacher, Rachael M., et al.
Publicado: (2026)
Driving asymmetric red supergiants winds with binary interactions
por: Landri, Camille, et al.
Publicado: (2024)
por: Landri, Camille, et al.
Publicado: (2024)
Photometric and spectroscopic variability of the blue supergiant rho Leo
por: Checha, V. A., et al.
Publicado: (2025)
por: Checha, V. A., et al.
Publicado: (2025)
Instabilities in models of supergiants MWC 137 and MWC 314
por: Parida, Sugyan, et al.
Publicado: (2024)
por: Parida, Sugyan, et al.
Publicado: (2024)
Multi epoch spectroscopic variability of the B supergiant HD75149
por: Chamoun-Contreras, J., et al.
Publicado: (2026)
por: Chamoun-Contreras, J., et al.
Publicado: (2026)
Magnetic field monitoring of four massive A-F supergiants
por: Wade, Gregg, et al.
Publicado: (2025)
por: Wade, Gregg, et al.
Publicado: (2025)
Modelling predicts a molecule-rich disk around the AGB star L2 Puppis
por: Van de Sande, M., et al.
Publicado: (2024)
por: Van de Sande, M., et al.
Publicado: (2024)
Hot and cool: Characterising the companions of red supergiant stars in binary systems
por: Patrick, L. R., et al.
Publicado: (2024)
por: Patrick, L. R., et al.
Publicado: (2024)
ALMA detection of CO rotational line emission in red supergiant stars of the massive young star cluster RSGC1 -- Determination of a new mass-loss rate prescription for red supergiants
por: Decin, Leen, et al.
Publicado: (2023)
por: Decin, Leen, et al.
Publicado: (2023)
Binarity at LOw Metallicity (BLOeM): The multiplicity properties and evolution of BAF-type supergiants
por: Patrick, L. R., et al.
Publicado: (2025)
por: Patrick, L. R., et al.
Publicado: (2025)
Properties of self-excited pulsations in 3D simulations of AGB stars and red supergiants
por: Ahmad, Arief, et al.
Publicado: (2022)
por: Ahmad, Arief, et al.
Publicado: (2022)
The Blue supergiant problem and the main-sequence width
por: Vink, Jorick S., et al.
Publicado: (2025)
por: Vink, Jorick S., et al.
Publicado: (2025)
Variability of Galactic blue supergiants observed with TESS
por: Kourniotis, Michalis, et al.
Publicado: (2025)
por: Kourniotis, Michalis, et al.
Publicado: (2025)
KIC 9272276: An Extreme Low Mass Ratio Red Nova Progenitor
por: Wadhwa, Surjit, et al.
Publicado: (2025)
por: Wadhwa, Surjit, et al.
Publicado: (2025)
The IACOB project: CVIII. Hunting for spectroscopic binaries in the O and B supergiant domain.The threat of pulsational variability
por: Simón-Díaz, S., et al.
Publicado: (2024)
por: Simón-Díaz, S., et al.
Publicado: (2024)
A phoenix rises from the ashes: WOH G64 is still a red supergiant, for now
por: van Loon, Jacco Th., et al.
Publicado: (2026)
por: van Loon, Jacco Th., et al.
Publicado: (2026)
Strong lithium lines in red supergiants at different metallicities
por: Negueruela, Ignacio, et al.
Publicado: (2022)
por: Negueruela, Ignacio, et al.
Publicado: (2022)
The circumstellar environment around the extreme Galactic red supergiant NML Cygni: Dense, dusty, and asymmetric
por: De Beck, E., et al.
Publicado: (2025)
por: De Beck, E., et al.
Publicado: (2025)
TESS light curves of two new magnetic cataclysmic variables: an asynchronous polar at the period minimum, and an eclipsing system with a large spin-to-orbit ratio
por: Littlefield, Colin, et al.
Publicado: (2026)
por: Littlefield, Colin, et al.
Publicado: (2026)
The evolution of accretor stars in binary systems due to accretion of increasingly helium-rich material
por: Richards, Sean, et al.
Publicado: (2024)
por: Richards, Sean, et al.
Publicado: (2024)
Stephenson 2 DFK 52: Discovery of an exotic red supergiant in the massive stellar cluster RSGC2
por: Siebert, Mark A., et al.
Publicado: (2025)
por: Siebert, Mark A., et al.
Publicado: (2025)
The Mass of the Vela Pulsar Progenitor and the Age of the Vela-Puppis Complex
por: Murphy, Jeremiah W., et al.
Publicado: (2024)
por: Murphy, Jeremiah W., et al.
Publicado: (2024)
Photometric and Spectroscopic study of Ten Low Mass Ratio Contact Binary Systems: Orbital Stability, O'Connell Effect and Infra-red Calcium Line Filling
por: Wadhwa, Surjit S., et al.
Publicado: (2024)
por: Wadhwa, Surjit S., et al.
Publicado: (2024)
Red supergiant stars in binary systems II. Confirmation of B-type companions of red supergiants in the Small Magellanic Cloud using Hubble ultra-violet spectroscopy
por: Patrick, L. R., et al.
Publicado: (2024)
por: Patrick, L. R., et al.
Publicado: (2024)
X-Shooting ULLYSES: Massive stars at low metallicity XV. On the metallicity dependence of B-supergiant mass-loss rates
por: Verhamme, O., et al.
Publicado: (2026)
por: Verhamme, O., et al.
Publicado: (2026)
High-resolution near-IR spectroscopy of the B[e] supergiant LHA 115-S 18: discovery of hot water vapor emission
por: Arias, M. L., et al.
Publicado: (2026)
por: Arias, M. L., et al.
Publicado: (2026)
Investigating the metallicity dependence of the mass-loss rate relation of red supergiants
por: Antoniadis, K., et al.
Publicado: (2025)
por: Antoniadis, K., et al.
Publicado: (2025)
MUSE 3D spectroscopy of BA-type supergiants in NGC 300
por: González-Torà, Gemma, et al.
Publicado: (2022)
por: González-Torà, Gemma, et al.
Publicado: (2022)
The red supergiant progenitor luminosity problem
por: Beasor, Emma R., et al.
Publicado: (2024)
por: Beasor, Emma R., et al.
Publicado: (2024)
Discoveries of fine structures and secondary pulses in coherent radio emission from a magnetic massive star
por: Das, Barnali, et al.
Publicado: (2025)
por: Das, Barnali, et al.
Publicado: (2025)
Investigating episodic mass loss in evolved massive stars IV. Comprehensive analysis of dusty red supergiants in NGC 6822, IC 10, and WLM
por: Christodoulou, E., et al.
Publicado: (2025)
por: Christodoulou, E., et al.
Publicado: (2025)
Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity
por: de Wit, S., et al.
Publicado: (2024)
por: de Wit, S., et al.
Publicado: (2024)
Ejemplares similares
-
Epsilon Sagittarii: An Extreme Rapid Rotator with a Decretion Disk
por: Bailey, Jeremy, et al.
Publicado: (2024) -
Polarization position angle standard stars: a reassessment of $θ$ and its variability for seventeen stars based on a decade of observations
por: Cotton, Daniel V., et al.
Publicado: (2024) -
Spectro Capture: A Software System for Automated Small-Observatory Spectroscopy
por: Luckas, Paul
Publicado: (2026) -
Observed epochal variations in X-ray lines from the O Supergiant $ζ$ Puppis do not require substantial changes in the wind mass flux
por: Gunderson, Sean J., et al.
Publicado: (2024) -
Absolute Parameters of Young Stars: NO Puppis
por: Erdem, Ahmet, et al.
Publicado: (2025)