Results 151 to 160 of about 45,569 (296)
Outflows from the youngest stars are mostly molecular. [PDF]
Ray TP+22 more
europepmc +1 more source
Comments on the Paper by A. E. Rydgren "T Tauri Stars and the (J-H), (H-K) Diagram" [PDF]
B. Baschek, R. Wehrsě
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Optical Monitoring of T Tauri Stars [PDF]
At the Van Vleck Observatory of Wesleyan University, Middletown, Connecticut, we have initiated a program of monitoring T Tauri stars with the 24-inch reflector (Perkin Telescope). During the first observing season, we have obtained UBVRI and Hα (30Å and 150Å) data for five stars: T Tau, RY Tau, SU Aur, RW Aur, and CO Ori.
openaire +2 more sources
Water in the terrestrial planet-forming zone of the PDS 70 disk. [PDF]
Perotti G+44 more
europepmc +1 more source
The Identification of T Tauri-Like Stars by Multicolour Photometry [PDF]
K. Nandy
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Properties of the Winds of T Tauri Stars [PDF]
The properties of Classical T Tauri (TTS) winds - their mass loss rate, temperature, origin, and energetics - are reviewed and interpreted in terms of the most recent observational evidence. TTS winds seem to have their origin in the disk and are powered by accretion. Most TTS have Ṁω ≤ 10–9Mʘ yr–1 and Ṁω/Ṁ ∼ 0.1, with T ∼ 104K.
openaire +2 more sources
We present results from simultaneous far-ultraviolet (FUV) and near-ultraviolet (NUV) observations of T Tauri stars (TTSs) in the Taurus molecular cloud with UVIT/AstroSat. This is the very first UVIT study of TTSs.
Prasanta K. Nayak+6 more
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Quasicyclic Light Changes in Three Low Mass T Tauri Stars [PDF]
H. Mauder
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X-Ray Observation on the Monoceros R2 Star-Forming Region with the Chandra ACIS-I Array
We report on the results of the Chandra observation on the central region of the Monoceros R2 cloud (Mon R2), a high-mass star-forming region (SFR). With a deep exposure of 100 ks, we detected 368 X-ray sources, 80% of which were identified with the NIR ...
Imanishi, Kensuke+4 more
core +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.
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