|
THE FLASH CODE AT INAF/OAPa
3-D Interaction of a SNR Shock and an Isolated Gas Cloud |
(Orlando et al. 2005, A&A 444, 505) |
| |
|
3-D visualizations of the mass density evolution during the shock-cloud
interaction. The movie shows the density distributions, in log scale.
click here to see the movie
|
| |
Crushing of interstellar gas clouds in supernova remnants:
X-ray emission
|
(Orlando et al. 2006, A&A 457, 545) |
| |
|
Evolution of the X-ray emission in the [0.1 - 10] keV band originating
from the shock-cloud interaction as derived from models with (model
RCm50c10) or without (model HYm50c10) thermal conduction and radiative
losses (see Fig. 4 in the paper). The
panel on the left shows the corresponding X-ray light curve of the cloud
(see Fig. 2 in the paper).
click here to see the movie
|
| |
On the origin of asymmetries in bilateral supernova remnants
|
(Orlando et al. 2007, A&A 470, 927) |
| |
|
Synchrotron radio emission (normalized to the maximum of each panel),
at t=18 kyrs, synthesized from models assuming a gradient of ambient
plasma density (panels A and D) or of ambient magnetic field strength
(panels B and E) when the LoS is aligned with the y axis. All the models
assume quasi-perpendicular particle injection. The directions of the
average unperturbed ambient magnetic field and of the plasma density or
magnetic field strength gradient are shown in the upper left and lower
right corners of each panel, respectively. The right panels show two
examples of radio maps (data adapted from Whiteoak & Green 1996 and
Gaensler 1998; the arrows point in the north direction) collected for
the SNRs G338.1+0.4 (panel C) and G296.5+10.0 (panel F). The color scale
is linear and is given by the bar on the right.
|
|
|
|
|