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Exploring the bow shock and beyond(图)     弓形冲击  天体物理  Rishabh·Datta       font style='font-size:12px;'> 2023/6/5
For most people, the night sky conjures a sense of stillness, an occasional shooting star the only visible movement. A conversation with Rishabh Datta, however, unveils the supersonic drama crashing a...
We present the discovery of strong mid-infrared emission lines of molecular hydrogen of apparently high-velocity dispersion (~870 km s-1) originating from a group-wide shock wave in Stephan's Quintet....
We conducted shock experiments simulating comet impacts to assess the feasibility of peptide synthesis by such a process. We used frozen mixture of the amino acid glycine, water ice, and silicate (fo...
Discerning the radiative dissipation mechanism for prompt emission in Gamma-Ray Bursts (GRBs) requires detailed spectroscopic modeling that straddles the $\nu F_{\nu}$ peak in the 100 keV - 1 MeV rang...
It is only now, with low-frequency radio telescopes, long exposures with high-resolution X-ray satellites and gamma-ray telescopes, that we are beginning to learn about the physics in the periphery of...
We present new Chandra X-ray and Giant Meterwave Radio Telescope (GMRT) radio observations of the nearby merging galaxy cluster Abell 754. Our X-ray data confirm the presence of a shock front by obtai...
An asymmetry between the ingress and egress times was observed in the near-UV light curve of the transit planet WASP-12b. Such asymmetry led us to suggest that the early ingress in the UV light curv...
Los trabajos que, junto con mi director, presentaremos a continuaci´on se engloban dentro de la tesis de doctorado titulada “Emisi´on no-t´ermica asociada a ondas de choque astrof&a...
Intergalactic shock fronts     High Energy Astrophysical Phenomena (astro-ph.HE)       font style='font-size:12px;'> 2011/1/7
When galaxy clusters collide, they generate shock fronts in the hot intracluster medium. Observations of these shocks can provide valuable information on the merger dynamics and physical conditions in...
We present a grid of nonequilibrium ionization models for the X-ray spectra from supernova remnants undergoing efficient diffusive shock acceleration. The calculation follows the hydrodynamics of the ...
Shock-in-jet model for quasars and microquasars     High Energy Astrophysical Phenomena (astro-ph.HE)       font style='font-size:12px;'> 2010/12/24
We present the theoretical background and detailed equations for the synchrotron emission of a shock wave propagating in a relativistic jet. We then show how the evolution of an outburst in this shock...
Possible saturation of betatron acceleration of dust particles behind strong shock fronts from supernovae is considered. It is argued that the efficiency of the nonthermal dust destruction should be s...
Fuse Observations of the Cygnus Loop:Probing Shock-Cloud Interactions。
The “Ghost Shell”:Discovery of the Forward Shock from Colliding Winds about Eta Carinae。
Tracing shock evolution in yso Jets     Tracing shock evolution  yso Jets       font style='font-size:12px;'> 2009/6/10
Tracing shock evolution in yso Jets。

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