Imagen de Portada

Do accretion-powered stellar winds help spin down T Tauri stars?

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Gehrig, Lukas, Gaidos, Eric, Venuti, Laura, Cody, Ann Marie, Turner, Neal J.
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

FitteR for Accretion ProPErties of T Tauri stars (FRAPPE): A new approach to use Class III spectra to derive stellar and accretion properties
por: Claes, R. A. B., et al.
Publicado: (2024)

The ODYSSEUS Survey. Using accretion and stellar rotation to reveal the star-disk connection in T Tauri stars
por: Pittman, Caeley V., et al.
Publicado: (2025)

Monitoring the magnetospheric accretion of the classical T Tauri star DO Tau with SPIRou
por: Donati, J. -F., et al.
Publicado: (2026)

Lithium and the evolution of intermediate-mass T Tauri and Herbig stars. Rotation, accretion, and planets
por: Mendigutía, I., et al.
Publicado: (2026)

The GRAVITY young stellar object survey -- XV. The star-disk interaction region of the T Tauri star DO Tau
por: GRAVITY Collaboration, et al.
Publicado: (2026)

Using the Ca II lines in T Tauri stars to infer the abundance of refractory elements in the innermost disk regions
por: Micolta, Marbely, et al.
Publicado: (2024)

SPIRou spectropolarimetry of the T Tauri star TW Hydrae: magnetic fields, accretion and planets
por: Donati, J. -F., et al.
Publicado: (2024)

Characterising the magnetospheric accretion process of DF Tauri's primary
por: Pouilly, K., et al.
Publicado: (2026)

Preparing for the Early eVolution Explorer: Characterizing the photochemical inputs and transit detection efficiencies of young planets using multiwavelength flare observations by TESS and Swift
por: Howard, Ward S., et al.
Publicado: (2024)

The classical T Tauri star CI Tau observed with SPIRou: magnetospheric accretion and planetary formation
por: Donati, J. -F., et al.
Publicado: (2024)

Circumstellar disk accretion across the Lagoon Nebula: the influence of environment and stellar mass
por: Venuti, L., et al.
Publicado: (2024)

Mass, Gas, and Gauss around a T Tauri Star with SPIRou
por: Donati, J. -F., et al.
Publicado: (2025)

The ODYSSEUS Survey. Characterizing magnetospheric geometries and hotspot structures in T Tauri stars
por: Pittman, Caeley V., et al.
Publicado: (2025)

Short- and long-term variations of the high mass accretion rate classical T Tauri star DR Tau
por: Zsidi, Gabriella, et al.
Publicado: (2025)

The optical photometric variability of Herbig Ae/Be stars from TESS
por: Cody, Ann Marie, et al.
Publicado: (2025)

High energy emission powered by accreting companions of Be/gamma Cas stars
por: Rast, Rina G., et al.
Publicado: (2025)

Simultaneous FUV and NUV observations of T Tauri stars with UVIT/AstroSat: probing accretion process in young stars
por: Nayak, Prasanta K., et al.
Publicado: (2024)

TESS Discovers a Second System of Transiting Exocomets in the Extreme Debris Disk of RZ Psc
por: Gibson, Adalyn, et al.
Publicado: (2025)

Unveiling stellar spin: Determining inclination angles in Be stars
por: Turis-Gallo, D., et al.
Publicado: (2025)

Spectroscopy of a sample of RV Tauri stars without IR excess
por: Pukitis, Karlis, et al.
Publicado: (2026)

Radial velocities of narrow emission line components in the spectra of T Tauri stars
por: Kiryukhina, V. A., et al.
Publicado: (2024)

Understanding Balmer Decrements in T Tauri stars in terms of Multiflow Magnetospheric Accretion
por: Patiño, Naiara, et al.
Publicado: (2026)

Long period modulation of the classical T Tauri star CI Tau: evidence for an eccentric close-in massive planet at 0.17 au
por: Manick, R., et al.
Publicado: (2024)

Signature of spin-down stalling in stellar magnetic activity. The case of the open cluster NGC 6811
por: Santos, Ângela R. G., et al.
Publicado: (2025)

Stellar wind parameters of massive stars in accretion-powered High Mass X-ray Binary Pulsars
por: Beskrovnaya, N., et al.
Publicado: (2025)

The mass distribution of clumpy accretion onto the nearby young star TW Hya
por: Ji, Tao, et al.
Publicado: (2025)

Preferential accretion of binary stars
por: Dalsgaard, Daniel, et al.
Publicado: (2025)

Impacts of stellar wind and supernovae on the star cluster formation: origins of extremely high N/O ratios and multiple stellar populations
por: Fukushima, Hajime, et al.
Publicado: (2024)

Protoplanetary disks around magnetized young stars with large-scale magnetic fields I: Steady-state solutions
por: Steiner, D., et al.
Publicado: (2025)

The GRAVITY Young Stellar Object survey -- IX. Spatially resolved kinematics of hot hydrogen gas in the star/disk interaction region of T Tauri stars
por: GRAVITY Collaboration, et al.
Publicado: (2022)

Probing accretion and stellar properties in the Orion Nebula with VLT/X-Shooter
por: Piscarreta, L., et al.
Publicado: (2025)

Measurement of interstellar extinction for classical T Tauri stars using far-UV H2 line fluxes
por: Fuhrmeister, B., et al.
Publicado: (2024)

Formation of Be stars via wind accretion: Case study on Black hole + Be star binaries
por: Li, Zhenwei, et al.
Publicado: (2025)

New line-driven wind mass-loss rates for OB stars with metallicities down to $0.01\,Z_\odot$
por: Krticka, Jiri, et al.
Publicado: (2025)

Evolution of the relation between the mass accretion rate and the stellar and disk mass from brown dwarfs to stars
por: Almendros-Abad, V., et al.
Publicado: (2024)

An accreting dwarf star orbiting the S-type giant star pi1 Gru
por: Montargès, M., et al.
Publicado: (2025)

The backreaction of stellar wobbling on accretion discs of massive protostars
por: Meyer, D. M. -A., et al.
Publicado: (2024)

PENELLOPE VII: Revisiting empirical relations to measure accretion luminosity
por: Fiorellino, E., et al.
Publicado: (2025)

The accretion burst of the massive young stellar object G323.46 -0.08
por: Wolf, V., et al.
Publicado: (2024)

C3PO V: Comoving stellar pairs indicate rotational spin-down drives the main-sequence Li-Dip
por: Sun, Qinghui, et al.
Publicado: (2025)