• No se han encontrado resultados

Bursting SN 1996cr's bubble: hydrodynamic and X ray modelling of its circumstellar medium

N/A
N/A
Protected

Academic year: 2020

Share "Bursting SN 1996cr's bubble: hydrodynamic and X ray modelling of its circumstellar medium"

Copied!
21
0
0

Texto completo

Loading

Figure

Figure 1. (Top) The radio light curve of SN 1996cr. All available data from 843 MHz to 89 GHz are shown (some of which is previously unpublished and will be presented in Bauer et al., in preparation)
Figure 2. The initial density profile of the SN ejecta and CSM, used as initial conditions in the hydrodynamic simulations
Figure 3. These panels depict the hydrodynamic evolution of various quantities: ejecta density (black); CSM density (blue); temperature (red); and fluid velocity (green)
Figure 4. The velocity of the SN forward shock during the evolution. It is extremely high (exceeding 20,0000 km/s) in the first few months, but then drops dramatically when the shock encounters the higher density shell, and the interaction region is highly
+5

Referencias

Documento similar

The number density of scalar dark matter particles would then be produced in the early stages of the Universe, by a freeze-in mechanism due to its very feeble coupling to the

Astrometric and photometric star cata- logues derived from the ESA HIPPARCOS Space Astrometry Mission.

The photometry of the 236 238 objects detected in the reference images was grouped into the reference catalog (Table 3) 5 , which contains the object identifier, the right

In addition to traffic and noise exposure data, the calculation method requires the following inputs: noise costs per day per person exposed to road traffic

Public archives are well-established through the work of the national archive services, local authority-run record offices, local studies libraries, universities and further

Keywords: iPSCs; induced pluripotent stem cells; clinics; clinical trial; drug screening; personalized medicine; regenerative medicine.. The Evolution of

In addition, precise distance determinations to Local Group galaxies enable the calibration of cosmological distance determination methods, such as supernovae,

Cu 1.75 S identified, using X-ray diffraction analysis, products from the pretreatment of the chalcocite mineral with 30 kg/t H 2 SO 4 , 40 kg/t NaCl and 7 days of curing time at