Results 231 to 240 of about 31,062 (274)
Kingdom-wide comparison reveals the evolution of diurnal gene expression in Archaeplastida. [PDF]
Nat Commun, 2019 Ferrari C +11 more
europepmc +1 more source
Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky
Gilbert E +35 more
europepmc +1 more source
T Tauri stars : Optical lucky imaging polarimetry of HL and XZ Tau
, 2010 M. V. Persson
openalex +1 more source
Flaring activity on the disk of Classical T Tauri Stars: effects on disk stability
, 2018 S. Colombo +7 more
openalex +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
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
openaire +1 more source
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.
openaire +1 more source
The observable characteristics of young solar-mass stars (T Tauri stars) are reviewed. Modern theoretical concepts and models of these stars are discussed briefly.
openaire +1 more source
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
openaire +1 more source
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
openaire +1 more source
Annual Review of Astronomy and Astrophysics, 1989
Les similarites et les differences entre les etoiles T Tauri et les etoiles de masses comparables durant leurs evolutions sont etudiees a partir d'etudes ...
openaire +1 more source
Les similarites et les differences entre les etoiles T Tauri et les etoiles de masses comparables durant leurs evolutions sont etudiees a partir d'etudes ...
openaire +1 more source