Results 81 to 90 of about 968 (218)
JWST-MIRI Spectroscopy of Warm Molecular Emission and Variability in the AS 209 Disk
We present MIRI Medium-resolution Spectrograph observations of the large, multi-gapped protoplanetary disk around the T Tauri star AS 209. The observations reveal hundreds of water vapor lines from 4.9–25.5 μ m toward the inner ∼1 au in the disk ...
Carlos E. Romero-Mirza+26 more
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Exiles and innovators: a survey of heretics in sixteenth‐century Europe
Abstract The links between exile and innovation have often been studied in the case of the twentieth century, but much less in the case of early modern Europe – an age of some political exiles and many religious ones. This essay focuses on what has been called ‘the Reformation of the Refugees’ in the early sixteenth century.
Peter Burke
wiley +1 more source
The classical T Tauri star (CTTS) stage is a critical phase of the star and planet formation process. In an effort to better understand the mass accretion processes, which can dictate future stellar evolution and planet formation, a multiepoch ...
John Wendeborn+19 more
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The enviroments of T Tauri stars
The environments of T Tauri stars are probably determined by the interaction of a stellar wind with matter which is falling toward a newly formed star. As shown by Ulrich, the steady infall of cool gas with angular momentum toward the star leads to a density distribution with rhoproportionalr/sup -1/2/ inside a radius r/sub d/ and rhoproportionalr/sup -
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SUMMARY Plant genetic transformation is essential for understanding gene functions and developing improved crop varieties. Traditional methods, often genotype‐dependent, are limited by plants' recalcitrance to gene delivery and low regeneration capacity.
Christopher Youngstrom+2 more
wiley +1 more source
Some resolutions on T Tauri stars [PDF]
This symposium is dedicated to the results of studies of flare stars. The necessity of the detailed analysis of observational data on flare stars follows from the very simple fact, that until now the theory has not found for the answer to the question: why the young stars of low luminosity are flaring.
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TIC 290061484: A Triply Eclipsing Triple System with the Shortest Known Outer Period of 24.5 Days
We have discovered a triply eclipsing triple-star system, TIC 290061484, with the shortest known outer period, P _out , of only 24.5 days. This “eclipses” the previous record set by λ Tauri at 33.02 days, which held for 68 yr.
V. B. Kostov+15 more
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T Tauri and FU Orionis Stars [PDF]
A great deal of information on the continuous radiation of T Tau- and similar type stars has been acquired. The cause of the ultraviolet and infrared excess emission is discussed. The possibility that the blue continuum may arise from numerous line emissions is considered.
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Ionization and heating by X-rays and cosmic rays*
High-energy radiation from the central T Tauri and protostars plays an important role in shaping protoplanetary disks and influences their evolution. Such radiation, in particular X-rays and extreme-ultraviolet (EUV) radiation, is predominantly generated
Güdel Manuel
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On the Variable Nebul of Hind (N.G.C. 1555) and Struve (N.G.C. 1554) in Taurus, and on the Nebulous Condition of the Variable Star T Tauri [PDF]
E. E. Barnard
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