Results 271 to 280 of about 45,569 (296)
Celebrating 30 years of science from the James Clerk Maxwell Telescope. [PDF]
R Soc Open Sci, 2017 Robson I, Holland WS, Friberg P.
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Binarity and Accretion in AGB Stars: HST/STIS Observations of UV Flickering in Y Gem. [PDF]
Astrophys J, 2018 Sahai R +5 more
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Laboratory unraveling of matter accretion in young stars. [PDF]
Sci Adv, 2017 Revet G +24 more
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Observational evidence for enhanced magnetic activity of superflare stars. [PDF]
Nat Commun, 2016 Karoff C +13 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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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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Astrophysics, 2003
The observable characteristics of young solar-mass stars (T Tauri stars) are reviewed. Modern theoretical concepts and models of these stars are discussed briefly.
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The observable characteristics of young solar-mass stars (T Tauri stars) are reviewed. Modern theoretical concepts and models of these stars are discussed briefly.
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