Astronomers using ALMA have confirmed a rare quasar pair, J2037-4537, in merging galaxies at redshift 5.7 (less than a billion years old), revealing that supermassive black holes become active when galaxies merge and funnel gas to their centers; these black holes, separated by thousands of light-years, will form a binary system in about 2.1 billion years, potentially emitting gravitational waves detectable by pulsar timing arrays.
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Two blazing quasars caught waltzing into a merger #ShortsAñadido:
Astronomers have confirmed [music] a rare quasar pair, J2037-4537, in merging galaxies [music] at redshift 5.7 using Alma. This discovery is one of only two quasar [music] pairs found at such an early stage of the universe, less than a billion years old. Quasars are powered by supermassive [music] black holes, which become active when galaxies merge and funnel gas to their centers. The research team mapped ionized carbon emission between the quasars, [music] revealing a tidal bridge confirming their merger. Each quasar host galaxy is massive with over 10 billion solar masses and star formation [music] rates above 500 solar masses per year.
Currently separated by thousands of light-years, these black holes will form a binary [music] system in about 2.1 billion years. Their eventual merger could emit gravitational [music] waves detectable by pulsar timing arrays, shedding light on cosmic phenomena. This discovery advances our understanding [music] of galaxy mergers, quasar activity, and the evolution of supermassive black holes. Future observations of quasar pairs like J2037-4537 will deepen insights into early universe dynamics and gravitational waves. Follow for [music] more news or visit the Upside Observer for the latest in positive news from around [music] the world.
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