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Our results constitute the most compelling evidence to date that young brown dwarfs undergo a T Tauri-like accretion phase similar to that in stars. A T-Tauri's heat is not generated by conversion but by the continual collapse of the area. Only when the star has sufficient mass to begin conversion that the next phase begins. T-Tauri was first discovered by John Russell Hind who was studying the night sky when he discovered a star that was no marked on any maps. This star was T-Tauri. おうし座T型星（おうしざテ（ィ）ーがたせい、T Tauri star, TTS）は、爆発型変光星の一種である。. 概説.

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Cite . BibTex; 2010-04-01 · T Tauri stars are pre-main sequence stars – the youngest visible F, G, K, M spectral type stars (<2 Solar mass).

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Se hela listan på de.wikipedia.org In the nonaccretors in our sample, Hα emission is commensurate with, or higher than, saturated levels in field M dwarfs of similar spectral type. Our results constitute the most compelling evidence to date that young brown dwarfs undergo a T Tauri-like accretion phase similar to that in stars. 2007-01-18 · T-Tauri is a variable star and is often used also to refer to a particular category of similar variable stars that are extremely young, pre-main sequence. I would guess that "T-Tauri phase" indicates a star that is in the same phase of life as T-Tauri, but without a better sense of the context for your question, it's hard to provide a complete answer.
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LGE T. Lange Ergebnisse von 48 Halbregelmäßigen und RV Tauri Sternen und 21 Die BR für Nebenminima wurden immer mit Phase 0,5. /J (indoeur.

så föreligger åtminstone en rent teoretisk möjlighet alt finna cornicis aevum, gloriam tauri trucis Phase, utg. genom Ludvig Larsson, häft. 1-2. The first phase of testing is done by This test is not based on any scientific study is to have his first Formula 1 test in an Alpha Tauri car at Imola on 4 November.
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The role of birthline age corrections, masses accreted during the T Tauri phase are roughly consistent with disk masses estimated from millimeter-wave dust emission.