We propose a full-track GMVA observation with GBT at 2 Gbps recording mode towards the M 87 jet. With this observation, we plan to define the structure, streamline, of the jet as is the same method as used in Asada &Nakamura 2012. We expect to see parabolic or conical streamline towards innermost jet region. Since the streamline of the jet is closely related to the acceleration mechanism of the jet, we can idenfity the initial acceleration mechanism either "magnetic centrifugal force dominate" or "magnetic pressure dominate".
Name | Institution |
---|---|
Masanori Nakamura | Academia Sinica; National Institute of Technology, Hachinohe College |
Juan Carlos Algaba | Academia Sinica; Korea Astronomy and Space Science Institute; Seoul National University |
Makoto Inoue | Academia Sinica |
Satoki Matsushita | Academia Sinica |
Nicolas Pradel | Academia Sinica; Auckland University of Technology |
Hiroaki Nishioka | Academia Sinica |
Cheng-Yu Kuo | Virginia, University of; National Sun Yat-sen University |
GBT Operator | Green Bank Observatory |
Keiichi Asada * | Academia Sinica |
* indicates the PI