We review the known properties of molecular outflows from low-and high-mass young stars.
General trends among outflows are identified, and the most recent studies on the …

We present small-scale 3D hydrodynamical simulations of the evolution of a 0.3 M⊙ main-
sequence (MS) star that launches two perpendicular jets within the envelope of a 0.88 M⊙ …

ABSTRACT We present Submillimeter Array observations toward the 10 4.7 L☉ star-forming
region G240. 31+ 0.07, in the J= 2–1 transition of 12 CO and 13 CO and at 1.3 mm …

“Cherchez le champ magnétique” is trendy in astronomy. The magnetic field takes the
hourglass shape in gravitationally contracting young stellar objects, helically wraps up the …

Studies of jets from young stellar objects (YSOs) suggest that material is launched from a
small central region at wide opening angles and collimated by an interaction with the …

New high-resolution molecular line and continuum millimeter interferometer observations of
the environment within 10 4 AU of the low-mass protostar IRAS 20582+ 7724, in the L1228 …

Steady-state, spherically symmetric accretion flows are well understood in terms of the Bondi
solution. Spherical symmetry, however, is necessarily an idealized approximation to reality …

We present new multiline and 3 mm continuum interferometer observations of the
circumstellar environment within 2× 10 4 AU of the class 0 protostar IRAS 05295+ 1247, the …

The thermal dust continuum emission at 848 μ m from the globule CB 068, a Class 0 young
stellar object (YSO), reveals strong linear polarization percentage values (up to 11%) in two …

Two three-dimensional magnetohydrodynamic simulations of strongly magnetized conical
jets, one with a poloidal and one with a helical magnetic field, have been performed. In both …