Context. The Taurus Molecular Cloud (TMC) is the nearest large star-forming region,
prototypical for the distributed mode of low-mass star formation. Pre-main sequence stars …

A method for following fragmentation simulations further in time using smoothed particle
hydrodynamics (SPH) is presented. In a normal SPH simulation of the collapse and …

We present new measurements of disk accretion rates for T Tauri stars in the Taurus
molecular cloud complex. Our results are based on intermediate-resolution …

We present a sensitive, multiwavelength submillimeter continuum survey of 153 young
stellar objects in the Taurus-Auriga star formation region. The submillimeter detection rate is …

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 …

We present the most sensitive 3 mm-survey to date of protoplanetary disks carried out in the
Taurus-Auriga star forming region (average rms of about 0.3 mJy), using the IRAM PdBI …

We present the results of a λ= 2.7 mm continuum interferometric survey of 24 young stellar
objects in 11 fields. The target objects range from deeply embedded class 0 sources to …

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 …

Context. Proto-planetary disks are thought to provide the initial environment for planetary
system formation. The dust and gas distribution and its evolution with time is one of the key …