Magnetospheric accretion models for T Tauri stars. 1: Balmer line profiles witho ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …

We present the results of a magnitude limited (K≤ 8.5 mag) multiplicity survey of T Tauri
stars (TTS) in two nearby star forming regions (SFR), Taurus-Auriga and Ophiuchus …

We present a high spatial resolution multiwavelength survey of 44 young binary star systems
in Taurus-Auriga with separations of 10–1000 AU. These observations, which were obtained …

▪ Abstract Accretion disks are important for many astrophysical phenomena, including
galactic nuclei, interacting binary stars, and young stellar objects. The central issue in the …

We surveyed all those young stars in the Taurus star forming region for duplicity which are
contained in the Herbig-Bell catalog and are brighter than K= 9.5 mag, in total a sample of …

We construct detailed vertical structure models of irradiated accretion disks around T Tauri
stars with interstellar medium dust uniformly mixed with gas. The dependence of the …

Scintillation is a well-known phenomenon in astronomy, eg twinkling of stars due to
scattering in the Earth's atmosphere, and variability of compact radio sources due to …

Coyotes-I - the Photometric Variability and Rotational Evolution of T-Tauri Star ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …

We present mid-infrared spectra of T Tauri stars in the Taurus star-forming region obtained
with the Spitzer Infrared Spectrograph (IRS). For the first time, the 5-36 μm spectra of a large …

The embedded young stars in the Taurus-Auriga molecular cloud. I - Models for sp ADS Classic
is now deprecated. It will be completely retired in October 2019. This page will automatically …