Physics
Scientific paper
Jan 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358..169u&link_type=abstract
In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 169-176 (SEE N85-17755 08-88)
Physics
Carbon Monoxide, Emission, Hot Stars, Jet Flow, Stellar Magnetic Fields, X Rays, Bipolarity, Simulation, Stellar Evolution, Stellar Gravitation, Stellar Models, Stellar Motions, Stellar Radiation, Stellar Structure
Scientific paper
Production of both the large scale CO bipolar flows and the small scale optical bipolar jets from the star-forming regions is given interpretation in terms of a magnetic mechanism related to accretion model. It is shown by an axisymmetric 2.5-dimensional simulation that the large scale cold bipolar flow may be produced in the relaxation of the magnetic twist which is created by the rotational winding-up of the magnetic field in the contracting disk. In contrast, the small scale warm bipolar jets may be driven by the recoiling shocks which are produced in the crash at the stellar surface of the infalling material released from the inner edge of the disk through magnetic reconnections.
Shibata Kazunari
Uchida Yoshiharu
No associations
LandOfFree
Bipolar flows and X-ray emission from young stellar object does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Bipolar flows and X-ray emission from young stellar object, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bipolar flows and X-ray emission from young stellar object will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-927332