Search Results - "Sarkar, Kartick Chandra"

Multiwavelength features of Fermi bubbles as signatures of a Galactic wind by Sarkar, Kartick Chandra, Nath, Biman B., Sharma, Prateek

“…Using hydrodynamical simulations, we show for the first time that an episode of star formation in the centre of the Milky Way, with a star formation rate (SFR)…”
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Long way to go: how outflows from large galaxies propagate through the hot halo gas by Sarkar, Kartick Chandra, Nath, Biman B., Sharma, Prateek, Shchekinov, Yuri

“…Using hydrodynamic simulations, we study the mass-loss due to supernova-driven outflows from Milky Way type disc galaxies, paying particular attention to the…”
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Possible connection between the asymmetry of North Polar Spur and Loop I with Fermi Bubbles by Sarkar, Kartick Chandra

“…The origin of North Polar Spur (NPS) and Loop-I has been debated over almost half a century and is still unresolved. Most of the confusion is caused by the…”
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Non-equilibrium ionisation and radiative transport in an evolving supernova remnant by Sarkar, Kartick Chandra, Gnat, Orly, Sternberg, Amiel

“…We present numerical simulations of the evolution of a supernova (SN) remnant expanding into a uniform background medium with density $n_H = 1.0$ cm$^{-3}$ and…”
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A new ionisation network and radiation transport module in PLUTO by Sarkar, Kartick Chandra, Sternberg, Amiel, Gnat, Orly

“…We introduce a new general-purpose time-dependent ionisation network (IN) and a radiation transport (RT) module in the magneto-hydrodynamic (MHD) code PLUTO…”
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Multi-wavelength features of Fermi Bubbles as signatures of a Galactic wind by Sarkar, Kartick Chandra, Nath, Biman B, Sharma, Prateek

“…Using hydrodynamical simulations, we show for the first time that an episode of star formation in the center of the Milky Way, with a star-formation-rate (SFR)…”
Get full text

Long way to go: how outflows from large galaxies propagate through the hot halo gas by Sarkar, Kartick Chandra, Nath, Biman B, Sharma, Prateek, Shchekinov, Yuri

“…Using hydrodynamic simulations, we study the mass loss due to supernova-driven outflows from Milky Way type disk galaxies, paying particular attention to the…”
Get full text