Fuente del cercano IR (Strom et al. 1976) que excita el ... Ubicada en Tauro a 140 pc. Luminosidad bolom trica de 30 Lsol. Embebida en n cleo denso (1000 AU) ...
B-Fields do not play a role in angular momentum transfer in a ... Saito, Kawabe, Kitamura&Sunada 1996. L1551 IRS5. Optical Jets. Snell, Loren, &Plambeck 1980 ...
A Study of the CO2 Absorption Feature at 15.2 m of Several Young Stellar Objects ... Infrared Spectrograph (IRS) Short-High Module. Spectra. Optical Depth Plots ...
Centimeter and Millimeter Observations of Very Young Binary and Multiple Systems ... J. M. Torrelles (IEEC, Spain), J. M. Girart (U. Barcelona, Spain) ...
... the cubic interpolated propagation (CIP) method (Yabe &Aoki ... 1-Torsional Alfven wave is generated at the disk surface and propagates up into the corona ...
Planetologia Extrasolare Cenni teorie formazione pianeti Extrasolari R.U. Claudi Le orbite dei pianeti sono quasi circolari e complanari I pianeti giganti si formano ...
Located at Taurus at 140 pc. Bolometric luminosity of 30 Lsun. Embedded in dense core (1000 AU) ... as circular polarization characteristics of southern source ...
Podemos descomponer la velocidad total de un astro en dos componentes: la velocidad radial (la componente a lo largo de la l nea de visi n) y la velocidad ...
(HST Public Pictures) X-ray binary (SS 433, Courtesy of Amy J. Mioduszewski) Nearby AGN ... UV/X-ray excitation scenarii would not give momentum flux as a T Tauri star ...