UCD Project: (Sub)Stellar object emission in Radio waves. This project allows to compute the Radio Emission produced by a given (sub)stellar object, which can be an Ultra-Cool Dwarf or stellar objects with bigger dimensions. The research is especially focused in the gyrosynchrotron emission caused by charged particles spiralling along the magnetic field lines of the (sub)stellar object. The objects studied in this project are objects with strong magnetic fields (eg: Bp > 1000 Gauss).
The model developed in this project is based on the pipeline described in:
C.Trigilio el al. (ESO 2004) [Appendix A]
A&A 418, 593–605 (2004)
DOI: 10.1051/0004-6361:20040060
2022 - Marc Rosanes Siscart (marcrosanes@gmail.com)
C/ Carles Collet, 7; Barcelona (08031); Catalonia
This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or any later version.
This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details.
You should have received a copy of the GNU General Public License along with this program. If not, see https://www.gnu.org/licenses/.
Approximate frequency range of application of the present model: [1.5 - 18 GHz]