▪ Abstract Recent advances in the understanding of the chemical processes that occur
during all stages of the formation of stars, from the collapse of molecular clouds to the …

▪ Abstract The physical conditions in molecular clouds control the nature and rate of star
formation, with consequences for planet formation and galaxy evolution. The focus of this …

We present a substantial extension of the millimeter (mm) wave continuum photometry
catalog for circumstellar dust disks in the Taurus star-forming region, based on a new" …

Recent discoveries of extrasolar planets and new direct evidence for protoplanetary disks
around young stars have had a major impact on our understanding of star and planet …

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 …

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 …

We present a complete 1.3 mm continuum mapping survey of the embedded young stellar
objects (YSOs) in the Taurus molecular cloud. We have also imaged several isolated Bok …

Protostars emit more x-rays, hard and soft, than young sunlike stars in more advanced
stages of formation. The x-ray emission becomes harder and stronger during flares. The …

We present 7-mm continuum observations of 14 low-mass pre-main-sequence stars in the
Taurus-Auriga star-forming region obtained with the Very Large Array with~ 15 resolution …

We report new interferometric observations of IRAS 04368+ 2557 (L1527) in 13 CO (J= 1–
0), C 18 O (J= 1–0), and 2.7 mm continuum emission using the Nobeyama Millimeter Array …