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Variability of the SiO thermal line emission toward the young L1448-mm outflow
Variability SiO emission L1448-mm outflow
2011/10/8
The detection of narrow SiO thermal emission toward young outflows has been proposed to be a signature of the magnetic precursor of C-shocks. Recent modeling of the SiO emission across C-shocks predic...
Origin of Molecular Outflow Determined from Thermal Dust Polarization
formation ISM jets and outflows magnetic fields polarization methods numerical
2010/11/9
The observational expectation of polarization measurements of thermal dust ra-diation is investigated to find information on molecular outflows based on magne-tohydrodynamical (MHD) and radiation tran...
Magnetic field structure in a high-mass outflow/disk system
Solar and Stellar Astrophysics (astro-ph.SR)
2011/1/7
To characterize the magnetic field structure of the outflow and core region within a prototypical high-mass star-forming region, we analyzed polarized CO(3-2) - for the first time observed with the Su...
The interaction of a yso outflow with the surrounding molecular cloud core
yso outflow interaction molecular cloud core
2009/7/10
The interaction of a yso outflow with the surrounding molecular cloud core。
H2 velocity structure in the molecular outflow dr 21
H2 velocity structure molecular outflow dr 21
2009/7/9
H2 velocity structure in the molecular outflow dr 21。
Standing Shocks around Black Holes and Estimation of Outflow Rates Santabrata Das & S. K.
accretion disk black hole physics outflows
2009/5/19
We self-consistently obtain shock locations in an accretion
flow by using an analytical method. One can obtain the spectral properties,
quasi-periodic oscillation frequencies and the outflowrates wh...