Results 81 to 90 of about 7,097 (207)
Rotational Velocities and Radii Estimates of Low-mass Pre-main-sequence Stars in NGC 2264
Investigating the angular momentum evolution of pre-main-sequence (PMS) stars provides important insight into the interactions between Sun-like stars and their protoplanetary disks, and the timescales that govern disk dissipation and planet formation. We
Laurin M. Gray +4 more
doaj +1 more source
Observational clues to the physics at the magnetosphere in young stellar objects
Classical T Tauri stars offer an excellent laboratory to study the accretion process and star-disk interaction, which define the transfer of mass and angular momentum in the system. The interaction takes place very close to the star, in a region of about
Alencar Silvia H. P.
doaj +1 more source
CSI 2264: Accretion process in classical T Tauri stars in the young cluster NGC 2264 [PDF]
Context. NGC 2264 is a young stellar cluster (~3 Myr) with hundreds of low-mass accreting stars that allow a detailed analysis of the accretion process taking place in the pre-main sequence. Aims.
Alencar, S. H. P. +14 more
core +5 more sources
Magnetospheric accretion on the fully convective classical T Tauri star DN Tau [PDF]
We report here results of spectropolarimetric observations of the classical T Tauri star DN Tau carried out (at 2 epochs) with ESPaDOnS at the Canada-France-Hawaii Telescope within the `Magnetic Protostars and Planets' programme. We infer that DN Tau, with a photospheric temperature of 3,950+-50 K, a luminosity of 0.8+-0.2 Lsun and a rotation period of
Donati, JF +9 more
openaire +5 more sources
Ferroelectric HZO Thin Films for FEFETs: Crystal Structure‐Device Performance Relationship
Crystal Structure of HZO Thin Films Methods of Thin Film Deposition 1T‐FeFET Design Influence on Ferroelectric Properties FeFET Applications Recent Advances and Challenges ORTHORHOMBIC HEARTBEAT. Abstract The rapid development of hafnium zirconium oxide (HZO) thin films has established ferroelectric field‐effect transistors (FeFETs) as strong ...
Harsha Ragini Aturi +2 more
wiley +1 more source
Variable X-Ray Emission of the Planet Hosting T Tauri Star CI Tau
We report results of Chandra X-ray observations of CI Tau, a young magnetically active classical T Tauri star for which previous studies have reported periodic variability attributed to a massive planet in a short-period orbit.
Stephen L. Skinner, Manuel Güdel
doaj +1 more source
Modeling T Tauri Winds from He I 10830 Profiles [PDF]
The high opacity of He I 10830 makes it an exceptionally sensitive probe of the inner wind geometry of accreting T Tauri stars. In this line blueshifted absorption below the continuum results from simple scattering of stellar photons, a situation which ...
Blandford R. D. +6 more
core +3 more sources
Star-disk interaction in classical T Tauri stars revealed using wavelet analysis [PDF]
Accepted for publication in A& ...
Lopez Santiago, J. +5 more
openaire +4 more sources
ABSTRACT Marine microbial communities are structured by a complex interplay of deterministic and stochastic processes, yet how these vary across latitudes remains poorly understood. Most long‐term microbial observatories are restricted to temperate regions, limiting our ability to assess latitudinal contrasts in microbial dynamics.
Pedro C. Junger +13 more
wiley +1 more source
Lyα Scattering Models Trace Accretion and Outflow Kinematics in T Tauri Systems
T Tauri stars produce broad Ly α emission lines that contribute ∼88% of the total UV flux incident on the inner circumstellar disks. Ly α photons are generated at the accretion shocks and in the protostellar chromospheres and must travel through ...
Nicole Arulanantham +20 more
doaj +1 more source

