Robert Lea is a science journalist in the U.K. whose articles have been published in Physics World, New Scientist, Astronomy Magazine, All About Space, Newsweek and ZME Science. He also writes about science communication for Elsevier and the European Journal of Physics.
Black HolesCould the remains of a 'dead' comet still be in the solar system? Astronomers are still searching 6 years laterBreaking space news, the latest updates on rocket launches, skywatching events and more!Receive email from us on behalf of our trusted partners or sponsorsSign up to our monthly entertainment newsletter to keep up with all our coverage of the latest sci-fi and space movies, tv shows, games and books.
Discover this week's must-see night sky events, moon phases, and stunning astrophotos. Sign up for our skywatching newsletter and explore the universe with us!Space.com's Sci-Fi Reader's Club. Read a sci-fi short story every month and join a virtual community of fellow science fiction fans!Using NASA's Hubble Space Telescope and Chandra X-ray Observatory, astronomers have hunted for"wandering" black holes drifting through dwarf galaxies. The discovery of these rogue black holes in such small galaxies could provide a"fossil record" that helps to explain how supermassive black holes grew to masses of millions or even billions of times that of the sun.has increasingly been discovering these cosmic titans already in place when the cosmos was less than 1 billion years old. That is problematic because the merger and feeding processes that are thought to explain supermassive black hole growthmay kick off with so-called"black hole seeds" that give a head start to these growth processes. These seeds, classified as either"heavy" or"light," have proved elusive in galaxies in the early universe.seeds predict that their signatures should be visible in dwarf galaxies in the local universe with total stellar masses of billions of times that of the sun. Theseprovide a unique laboratory for studying black hole formation and early evolution, thanks to their relatively quiet merger histories compared to those of massive galaxies. This means they can provide a"fossil record" of the original black hole seeds via their non-central intermediate black holes.James Webb Space Telescope's mysterious 'little red dots' may be black holes in disguise A black hole 'feeding frenzy' could help explain a cosmic mystery uncovered by the James Webb Space Telescope, or they can be ravenously feeding on surrounding gas and dust, creating a violent and turbulent environment which astronomers call anThe team behind this investigation points out that the vast majority of black holes found in dwarf galaxies are accreting and have been identified as dwelling in AGNs. "Compared to more massive galaxies, dwarf galaxies can have lower central stellar densities and more irregularly shaped potential wells," team leader Megan R. Sturm of Montana State University told Space.com."As a result, if a black hole forms in the outer reaches of its host galaxy, it is unlikely to ever spiral down into the center. Some researchers have even predicted that approximately half of all black holes in dwarf galaxies are wandering. "If this is the case, all-sky surveys pointed at the centers of galaxies may simply be missing a large population of dwarf galaxies hosting massive black holes. This has important implications for black hole fraction in this mass range and, therefore, black hole formation through seeding."Breaking space news, the latest updates on rocket launches, skywatching events and more!Receive email from us on behalf of our trusted partners or sponsorsThe problem with detecting wandering black holes in these small galaxies is the fact that these dwarf galaxy AGNs have to be distinguished from other radiation sources, such as regions of intense star formation or"starbursts," and from"Observing massive black holes in the dwarf regime can be a complicated process. Since the maximum luminosity of an AGN is proportional to its mass, AGNs in dwarf galaxies are generally dimmer than their higher mass counterparts," Sturm said."Additionally, low-luminosity/ low-mass AGNs can lack a traditional broad line region or have broad lines that are weak and hard to detect. This makes them both harder to see and easier to confuse with other stellar objects or star-formation-related processes."to study 12 dwarf galaxies in which AGNs had previously been detected in radio waves. Eight of these AGNs appeared to be offset from the centers of their dwarf galaxy-hosts, or"non-nuclear," indicating they could harbor wandering black holes.James Webb Space Telescope's mysterious 'little red dots' may be black holes in disguise A black hole 'feeding frenzy' could help explain a cosmic mystery uncovered by the James Webb Space Telescope "Generally, supermassive black holes reside in the nucleus of massive galaxies. However, eight of the dwarf galaxies in our sample displayed compact radio emission originating from outside of the optical nucleus of the galaxy, offset by around one to two kiloparsecs and in some cases outside of the host galaxy entirely," Sturm said."These are potentially 'wandering' black hole candidates. While these wandering AGN candidates had been observed at radio frequencies, obtaining AGN-like observations at optical or X-ray wavelengths would confirm the presence of an AGN." Sturm explained that she and her colleagues were able to detect one of these sources, designated ID 64, in optical light with Hubble and in X-rays with Chandra. However, this revealed that it is actually a much more distant AGN that simply aligns with this dwarf galaxy from our perspective. "Seven galaxies in our sample do not have significantly detected optical/X-ray counterparts. However, it remains a possibility that these are wandering black holes that are either isolated or residing within globular or nuclear star clusters that are simply below our Hubble detection limits," she continued."It also remains a possibility that they are background, high-redshift interlopers that happen to overlap with our galaxies in the sky, such as the case for ID 64." Determining if these seven galaxies do indeed host wandering black holes or if these radio signals are the result of more distant AGNs could involve enlisting the help of the JWST, the $10 billion space telescope sibling of Hubble. "Identifying the origin of the off-nuclear radio sources for the remaining seven wandering black hole candidates may be possible with the exquisite capabilities of the JWST," Sturm said."With higher resolution, JWST could potentially observe the source of the compact radio emission, whether it be the core of a disrupted dwarf galaxy/star cluster within the host galaxy or a background, high-redshift galaxy." Robert Lea is a science journalist in the U.K. whose articles have been published in Physics World, New Scientist, Astronomy Magazine, All About Space, Newsweek and ZME Science. He also writes about science communication for Elsevier and the European Journal of Physics. Rob holds a bachelor of science degree in physics and astronomy from the U.K.’s Open University. Follow him on Twitter @sciencef1rst.'Good Luck, Have Fun, Don't Die' feels like '12 Monkeys' meets 'Shaun of the Dead' and a whole lot of AI dread
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