The Magnetoviscous-Thermal Instability

@inproceedings{Islam2011TheMI,
  title={The Magnetoviscous-Thermal Instability},
  author={Tajmeri Selima Akhter Islam},
  year={2011}
}
Accretion flows onto underluminous black holes, such as Sagittarius A* at the center of our galaxy, are dilute (mildly collisional to highly collisionless), optically thin, and radiatively inefficient. Therefore, the accretion properties of such dilute flows are expected to be modified by their large viscosities and thermal conductivities. Second… CONTINUE READING