40 citations · 80 across the 5 of their papers we have counts for
5 papers
Collapse of Turbulent Cores and Reconnection Diffusion
M. R. M. Leão, E. M. de Gouveia Dal Pino, R. Santos-Lima +1
For a molecular cloud clump to form stars some transport of magnetic flux is required from the denser, inner regions to the outer regions of the cloud, otherwise this can prevent t…
Magnetic Flux Transport by turbulent reconnection in astrophysical flows
Elisabete M. de Gouveia Dal Pino, Márcia R. M. Leão, Reinaldo Santos-Lima +3
The role of MHD turbulence in astrophysical environments is still highly debated. An important question that permeates this debate is the transport of magnetic flux. This is partic…
MHD turbulence-Star Formation Connection: from pc to kpc scales
E. M. de Gouveia Dal Pino, R. Santos-Lima, A. Lazarian +3
The transport of magnetic flux to outside of collapsing molecular clouds is a required step to allow the formation of stars. Although ambipolar diffusion is often regarded as a key…
Local Star formation triggered by SN shocks in magnetized diffuse neutral clouds
M. R. M. Leao, E. M. de Gouveia Dal Pino, D. Falceta-Goncalves +2
In this work, considering the impact of a SNR with a neutral magnetized cloud we derived analytically a set of conditions which are favorable for driving gravitational instability…
Star formation triggered by SNR impact into magnetized neutral clouds
M. R. M. Leao, E. M. de Gouveia Dal Pino, D. Falceta-Goncalves +2
Considering the physical conditions that are relevant for triggering star formation in interactions involving SN shocks and neutral clouds, we have built diagrams of the SNR radius…