23 citations · 37 across the 3 of their papers we have counts for
6 papers
Magnetic Field Orientation in Self-Gravitating Turbulent Molecular Clouds
Lucas Barreto-Mota, Elisabete M. de Gouveia Dal Pino, Blakesley Burkhart +3
Stars form inside molecular cloud filaments from the competition of gravitational forces with turbulence and magnetic fields. The exact orientation of these filaments with the magn…
Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
The Cherenkov Telescope Array Consortium, :, A. Acharyya +449
We provide an updated assessment of the power of the Cherenkov Telescope Array (CTA) to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray sig…
Diffusion of large-scale magnetic fields by reconnection in MHD turbulence
R. Santos-Lima, G. Guerrero, E. M. de Gouveia Dal Pino +1
The rate of magnetic field diffusion plays an essential role in several astrophysical plasma processes. It has been demonstrated that the omnipresent turbulence in astrophysical me…
A hadronic emission model for black hole-disc impacts in the blazar OJ 287
J. C. Rodríguez-Ramírez, P. Kushwaha, E. M. de Gouveia Dal Pino +1
A super-massive black hole (SMBH) binary in the core of the blazar OJ 287 has been invoked in previous works to explain its observed optical flare quasi-periodicity. Following this…
Magnetic fields in early protostellar disk formation
Diego F. González-Casanova, Reinaldo Santos-Lima, Alexander Lazarian
We consider formation of accretion disks from a realistically turbulent molecular gas using 3D MHD simulations. In particular, we analyze the effect of the fast turbulent reconnect…
Particle Acceleration by Magnetic Reconnection in AGNs and in the IGM
Elisabete M. de Gouveia Dal Pino, Grzegorz Kowal, Alex Lazarian +1
There is no single mechanism by which fast particles are accelerated in astrophysical environments, and it is now recognized that the data require a rich variety of different mecha…