Jets from Accreting Magnetic Young Stellar Objects. I. Comparison of Observations and High‐Resolution Simulation Results

1999 ◽  
Vol 524 (1) ◽  
pp. 142-158 ◽  
Author(s):  
Anthony P. Goodson ◽  
Karl‐Heinz Bohm ◽  
Robert M. Winglee
2020 ◽  
Vol 900 (2) ◽  
pp. 104
Author(s):  
Andrew G. Barr ◽  
Adwin Boogert ◽  
Curtis N. DeWitt ◽  
Edward Montiel ◽  
Matthew J. Richter ◽  
...  

2018 ◽  
Vol 14 (S343) ◽  
pp. 355-356
Author(s):  
Dylan Bollen ◽  
Devika Kamath ◽  
Hans Van Winckel ◽  
Orsola De Marco

AbstractWe have discovered jets in post-AGB binaries. The orbital motion allows us to carry out tomography of the jet as light from the primary star shines through the jet cone. Jets play a major role in many astrophysical environments, from young stellar objects to galaxies. They are also used to study the energetics of accretion phenomena in systems such as red transients and stellar mergers. We use high-resolution, optical, time-series spectra to constrain theories of jet launching, and the impact of jets on the evolution of these post-AGB binaries.


2008 ◽  
Vol 381-382 ◽  
pp. 509-512 ◽  
Author(s):  
Wen Wang ◽  
X.X. Li ◽  
Zi Chen Chen

A planar capacitive sensor (PCS) is proposed for X and Y directions measurement. One axial displacement can be measured without the coupling of another axial movement. Two groups electrodes with 90 degree out-of-phase, forming triangle sine and triangle cosine wave, can be applied for direction detection and interpolation, aiming at high resolution. Simulation results show that proposed PCS is available for planar measurement.


2002 ◽  
Vol 392 (3) ◽  
pp. 945-954 ◽  
Author(s):  
T. Preibisch ◽  
Y. Y. Balega ◽  
D. Schertl ◽  
G. Weigelt

2012 ◽  
Vol 747 (2) ◽  
pp. 142 ◽  
Author(s):  
G. G. Sacco ◽  
E. Flaccomio ◽  
I. Pascucci ◽  
F. Lahuis ◽  
B. Ercolano ◽  
...  

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