Complementing data with NASA's Chandra X-Ray Observatory provided additional insights.
can reheat the gas that surrounds it by sending out violent outbursts from its center. This process, called feedback, can prevent the cooling down of the atmosphere and the subsequent formation of a star.Jets of radiation that are part of the feedback from a supermassive black hole can carve out large cavities inside the hot plasma of the galaxy clusters. As the gas moves farther from the cluster center, it is replaced by large bubbles that can emit radiation, the press release said.
During their observation, the researchers used the Sunyaev-Zeldovich effect, which looks at the subtle distortion in the cosmic microwave background radiation due to scattering by hot electrons in the gas of a. The CMB was emitted 380,000 years thousand years after the Big Bang. The SZ effect signal as observed by the MUSTANG-2 receivers on the GBT telescope primarily measures thermal pressure, the press release said.NASA Chandra X Ray Observatory & the NSF's Green Bank Observatory.
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