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|    ScienceDaily to All    |
|    New discovery sheds light on very early     |
|    24 Feb 23 21:30:28    |
      MSGID: 1:317/3 63f98eec       PID: hpt/lnx 1.9.0-cur 2019-01-08       TID: hpt/lnx 1.9.0-cur 2019-01-08        New discovery sheds light on very early supermassive black holes                Date:        February 24, 2023        Source:        Royal Astronomical Society        Summary:        Astronomers have discovered a rapidly growing black hole in one        of the most extreme galaxies known in the very early Universe. The        discovery of the galaxy and the black hole at its center provides        new clues on the formation of the very first supermassive black        holes.                      Facebook Twitter Pinterest LinkedIN Email       FULL STORY       ==========================================================================       Astronomers from the University of Texas and the University of Arizona       have discovered a rapidly growing black hole in one of the most extreme       galaxies known in the very early Universe. The discovery of the galaxy       and the black hole at its centre provides new clues on the formation of       the very first supermassive black holes. The new work is published in       Monthly Notices of the Royal Astronomical Society.                     ==========================================================================       Using observations taken with the Atacama Large Millimeter Array (ALMA),       a radio observatory sited in Chile, the team have determined that the       galaxy, named COS-87259, containing this new supermassive black hole is       very extreme, forming stars at a rate 1000 times that of our own Milky       Way and containing over a billion solar masses worth of interstellar       dust. The galaxy shines bright from both this intense burst of star       formation and the growing supermassive black hole at its centre.              The black hole is considered to be a new type of primordial black hole       -- one heavily enshrouded by cosmic "dust," causing nearly all of its       light to be emitted in the mid-infrared range of the electromagnetic       spectrum. The researchers have also found that this growing supermassive       black hole (frequently referred to as an active galactic nucleus) is       generating a strong jet of material moving at near light speed through       the host galaxy.              Today, black holes with masses millions to billions of times greater than       that of our own Sun sit at the centre of nearly every galaxy. How these       supermassive black holes first formed remains a mystery for scientists,       particularly because several of these objects have been found when the       Universe was very young.              Because the light from these sources takes so long to reach us, we see       them as they existed in the past; in this case, just 750 million years       after the Big Bang, which is approximately 5% of the current age of       the Universe.              What is particularly astonishing about this new object is that it was       identified over a relatively small patch of the sky typically used to       detect similar objects -- less than 10 times the size of the full moon --       suggesting there could be thousands of similar sources in the very early       Universe. This was completely unexpected from previous data.              The only other class of supermassive black holes we knew about in the       very early Universe are quasars, which are active black holes that are       relatively unobscured by cosmic dust. These quasars are extremely rare       at distances similar to COS-87259, with only a few tens located over the       full sky. The surprising discovery of COS-87259 and its black hole raises       several questions about the abundance of very early supermassive black       holes, as well as the types of galaxies in which they typically form.              Ryan Endsley, the lead author of the paper and now a Postdoctoral Fellow       at The University of Texas at Austin, says "These results suggest that       very early supermassive black holes were often heavily obscured by dust,       perhaps as a consequence of the intense star formation activity in their       host galaxies. This is something others have been predicting for a few       years now, and it's really nice to see the first direct observational       evidence supporting this scenario." Similar types of objects have been       found in the more local, present-day Universe, such as Arp 299 shown       here. In this system, two galaxies are crashing together generating an       intense starburst as well as heavy obscuration of the growing supermassive       black hole in one of the two galaxies.              Endsley adds, "While nobody expected to find this kind of object in the       very early Universe, its discovery takes a step towards building a much       better understanding of how billion solar mass black holes were able to       form so early on in the lifetime of the Universe, as well how the most       massive galaxies first evolved."        * RELATED_TOPICS        o Space_&_Time        # Black_Holes # Galaxies # Astrophysics # Astronomy #        Stars # Cosmology # Big_Bang # Solar_System        * RELATED_TERMS        o Spitzer_space_telescope o Black_hole o Galaxy o        Holographic_Universe o Galaxy_formation_and_evolution o Quasar        o Edwin_Hubble o Black_body              ==========================================================================       Story Source: Materials provided by Royal_Astronomical_Society. Note:       Content may be edited for style and length.                     ==========================================================================       Journal Reference:        1. Ryan Endsley, Daniel P Stark, Jianwei Lyu, Feige Wang, Jinyi Yang,        Xiaohui Fan, Renske Smit, Rychard Bouwens, Kevin Hainline, Sander        Schouws. ALMA confirmation of an obscured hyperluminous radio-loud        AGN at z = 6.853 associated with a dusty starburst in the 1.5 deg2        COSMOS field.               Monthly Notices of the Royal Astronomical Society, 2023; 520 (3):        4609 DOI: 10.1093/mnras/stad266       ==========================================================================              Link to news story:       https://www.sciencedaily.com/releases/2023/02/230224135116.htm              --- up 51 weeks, 4 days, 10 hours, 50 minutes        * Origin: -=> Castle Rock BBS <=- Now Husky HPT Powered! 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