Results 41 to 50 of about 58,006 (237)
LIGHT CURVE TYPES OF CLASSIC T TAURI STARS
By using the archive photometric data’s obtained for a long time intervals we have carried out a master light curves of 28 classical T Tauri type stars. For the physical character of variability mainly 5 type light curves can be separated.
N. Z. Ismailov, H. N. Adygezalzade
doaj +1 more source
Large Myr-old Disks Are Not Severely Depleted of Gas-phase CO or Carbon
We present an ACA search for [C i ] 1–0 emission at 492 GHz toward large T Tauri disks (gas radii ≳ 200 au) in the ∼1–3 Myr-old Lupus star-forming region. Combined with Atacama Large Millimeter/submillimeter Array 12 m archival data for IM Lup, we report
Ilaria Pascucci+8 more
doaj +1 more source
Another deep dimming of the classical T Tauri star RW Aurigae A [PDF]
Context. RWAur A is a classical T Tauri star (CTTS) with an unusually rich emission line spectrum. In 2014 the star faded by similar to 3 mag in the V band and went into a long-lasting minimum.
P. Petrov+5 more
semanticscholar +1 more source
Inner disk structure of the classical T Tauri star LkCa 15 [PDF]
Context. Magnetospheric accretion has been thoroughly studied in young stellar systems with full non-evolved accretion disks, but it is poorly documented for transition disk objects with large inner cavities. Aims.
S. Alencar+17 more
semanticscholar +1 more source
Oscillations of the Boundary Layer and High-frequency QPOs
We observed persistent high-frequency oscillations of the boundary layer near an accreting, weakly-magnetized star in global 3D MHD simulations. The tilted dipole magnetic field is not strong enough to open a gap between the star and the disk.
Blinova A. A.+2 more
doaj +1 more source
A LAMOST Spectroscopic Study of T Tauri Stars in the Orion OB1a Subassociation
We present a spectroscopic analysis of T Tauri stars (TTSs) observed with the wide-field multifiber spectrograph LAMOST in the substellar associations Ori OB1a located in the Orion Star-forming Complex.
Jesús Hernández+11 more
doaj +1 more source
Observational Constraints on the Formation and Evolution of Binary Stars [PDF]
We present a high spatial resolution UV to NIR survey of 44 young binary stars in Taurus with separations of 10-1000 AU. The primary results include: (1) The relative ages of binary star components are more similar than the relative ages of randomly ...
A. M. Ghez+37 more
core +3 more sources
Magnetospheric accretion on the T Tauri star BP Tauri [PDF]
From observations collected with the ESPaDOnS and NARVAL spectropolarimeters, we report the detection of Zeeman signatures on the classical T Tauri star BP Tau.
J. Donati+17 more
semanticscholar +1 more source
MAGNETOSPHERIC ACCRETION IN T TAURI STARS: OBSERVATIONAL TEST
In the classical T Tauri stars (CTTS) the magnetic field plays an important role in the interaction between the star and the accretion disk. In 1996-2000 we have carried out an extensive spectroscopic and photometric monitoring of the extremly active ...
P. P. Petrov
doaj +1 more source
Magnetic fields and accretion flows on the classical T Tauri star V2129 Oph [PDF]
From observations collected with the ESPaDOnS spectropolarimeter, we report the discovery of magnetic fields at the surface of the mildly accreting classical T Tauri star V2129 Oph.
J. Donati+10 more
semanticscholar +1 more source