Results 181 to 190 of about 58,260 (304)

Multiplicity among T Tauri stars in OB and T associations: Implications for binary star formation

open access: green, 1995
W. Brandner   +4 more
openalex   +2 more sources

MINDS. JWST/MIRI Reveals a Dynamic Gas-rich Inner Disk inside the Cavity of SY Cha

open access: yesThe Astrophysical Journal
SY Cha is a T Tauri star surrounded by a protoplanetary disk with a large cavity seen in the millimeter continuum but has the spectral energy distribution of a full disk.
Kamber R. Schwarz   +25 more
doaj   +1 more source

Bringing high spatial resolution to the far-infrared: A giant leap for astrophysics. [PDF]

open access: yesExp Astron (Dordr), 2021
Linz H   +20 more
europepmc   +1 more source

The outburst of the T Tauri star EX Lupi in 1994

open access: green, 1995
Thomas Lehmann, Bo Reipurth, W. Brandner
openalex   +2 more sources

XMM-Newton spectroscopy of the metal depleted T Tauri star TWA 5 [PDF]

open access: bronze, 2005
C. Argiroffi   +4 more
openalex   +1 more source

Dispersed T Tauri stars and galactic star formation

open access: yesAIP Conference Proceedings, 1996
The spatial distribution, age distribution and kinematics of T Tauri stars, both close to and widely distributed around active clouds, are considered using simple models of T Tauri dispersal. Models are compared to observations in and around the nearby cloud complexes, in particular the recent discovery of widely scattered young stars from the ROSAT ...
openaire   +3 more sources

Grand Design Spiral Arms in the Compact, Embedded Protoplanetary Disk of Haro 6-13

open access: yesThe Astrophysical Journal
Millimeter continuum spiral arms have so far only been detected in a handful of protoplanetary disks, and thus we have a limited understanding of the circumstances in which they can form.
Jane Huang   +8 more
doaj   +1 more source

Rotational Evolution of Classical T Tauri Stars: Models and Observations

open access: yesThe Astrophysical Journal
We developed a grid of stellar rotation models for low-mass and solar-type classical T Tauri stars (CTTS; 0.3 M _⊙ < M _* < 1.2 M _⊙ ). These models incorporate the star–disk interaction and magnetospheric ejections to investigate the evolution of the ...
Javier Serna   +19 more
doaj   +1 more source

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