Results 211 to 220 of about 44,019 (234)
Ostreococcus tauri is a new model green alga for studying iron metabolism in eukaryotic phytoplankton. [PDF]
Lelandais G+13 more
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IRAS observations of T Tauri and post-T Tauri stars
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Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky
Gilbert E+35 more
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Hydroxyl super rotors from vacuum ultraviolet photodissociation of water. [PDF]
Chang Y+16 more
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Physics Reports, 1984
Abstract The observational aspects of T Tau stars are described, treating data in the optical, infrared, radio, X-ray and ultraviolet regions of the spectrum. Erratic flare-like behaviour is very characteristic of these objects which are pre-main-sequence stars, mostly on their convective tracks, and represent early phases in the evolution of roughly
Martin Cohen, Martin Cohen
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Abstract The observational aspects of T Tau stars are described, treating data in the optical, infrared, radio, X-ray and ultraviolet regions of the spectrum. Erratic flare-like behaviour is very characteristic of these objects which are pre-main-sequence stars, mostly on their convective tracks, and represent early phases in the evolution of roughly
Martin Cohen, Martin Cohen
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Spatially resolved magnetic field structure in the disk of a T Tauri star
Nature, 2014Magnetic fields in accretion disks play a dominant part during the star formation process but have hitherto been observationally poorly constrained. Field strengths have been inferred on T Tauri stars and possibly in the innermost part of their accretion
I. Stephens+10 more
semanticscholar +1 more source
Astrophysics and Space Science, 1998
A T Tauri Star Database was set up with the purpose of designing a user-friendly, graphical database which would provide a quick look into the properties of T Tauri stars.
J. F. Gameiro+2 more
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A T Tauri Star Database was set up with the purpose of designing a user-friendly, graphical database which would provide a quick look into the properties of T Tauri stars.
J. F. Gameiro+2 more
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Naked T Tauri stars and post T Tauri stars
2008It has become evident during the past few years that there is more to low mass pre-main sequence (PMS) stellar populations than the classical T Tauri stars (TTS). If all low mass stars pass through the T Tauri phase, and star formation continues for a dynamical timescale, then in a typical star formation region the post-T Tauri (PTT), PMS stars should ...
F. M. Walter, P. C. Myers
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