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Stellar feedback -- stars regulating further star formation through the injection of energy and momentum into the interstellar medium -- operates through a complex set of processes that originate in star clusters but shape entire galaxies. A mature theory of stellar feedback is essential to a complete theory of star and galaxy formation, but the energy and momentum injected by hot gas into its surroundings remains unclear. With a next-generation X-ray observatory, breakthrough progress can be made through precision measurements of the temperature, density, velocity, and abundances of hot gas on scales of star clusters to galactic superwinds.
We observe the 1.2 mm continuum emission around the OB cluster forming region G10.6-0.4, using the IRAM 30m telescope MAMBO-2 bolometer array and the Submillimeter array. Comparison of the Spitzer 24 $mu$m and 8 $mu$m images with our 1.2 mm continuum
The observed massive end of the galaxy stellar mass function is steeper than its predicted dark matter halo counterpart in the standard $Lambda $CDM paradigm. In this paper, we investigate the impact of active galactic nuclei (AGN) feedback on star f
We simulate the effects of massive star feedback, via winds and SNe, on inhomogeneous molecular material left over from the formation of a massive stellar cluster. We use 3D hydrodynamic models with a temperature dependent average particle mass to mo
We report the systematic analysis of knots, hotspots, and lobes in 57 active galactic nuclei (AGNs) to investigate the variation of the magnetic field along with the jet from the sub-pc base to the terminus in kpc-to-Mpc scales. Expanding the number
We investigated the jet width profile with distance along the jet in the nearby radio galaxy NGC 1052 at radial distances between $sim300$ to $4 times 10^7$ Schwarzschild Radii($R_{rm S}$) from the central engine on both their approaching and recedin