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|    ScienceDaily to All    |
|    Astronomers discover metal-rich galaxies    |
|    27 Feb 23 21:30:28    |
      MSGID: 1:317/3 63fd836c       PID: hpt/lnx 1.9.0-cur 2019-01-08       TID: hpt/lnx 1.9.0-cur 2019-01-08        Astronomers discover metal-rich galaxies in early universe                Date:        February 27, 2023        Source:        Cornell University        Summary:        While analyzing data from the first images of a well-known        early galaxy taken by NASA's James Webb Space Telescope (JWST),        astronomers discovered a companion galaxy previously hidden behind        the light of the foreground galaxy -- one that surprisingly seems        to have already hosted multiple generations of stars despite its        young age, estimated at 1.4 billion years old.                      Facebook Twitter Pinterest LinkedIN Email       FULL STORY       ==========================================================================       While analyzing data from the first images of a well-known early galaxy       taken by NASA's James Webb Space Telescope (JWST), Cornell University       astronomers discovered a companion galaxy previously hidden behind the       light of the foreground galaxy -- one that surprisingly seems to have       already hosted multiple generations of stars despite its young age,       estimated at 1.4 billion years old.                     ==========================================================================       "We found this galaxy to be super-chemically abundant, something none of       us expected," said Bo Peng, a doctoral student in astronomy, who led the       data analysis. "JWST changes the way we view this system and opens up new       venues to study how stars and galaxies formed in the early universe."       Peng is the lead author of "Discovery of a Dusty, Chemically Mature       Companion to z~4 Starburst Galaxy in JWST Early Release Science Data,"       published in theAstrophysical Journal Letters.              Earlier images captured by the Atacama Large Millimeter/submillimeter       Array (ALMA) in Chile contained hints of the companion resolved clearly       by JSWT, but couldn't be interpreted as anything more than random noise,       said Amit Vishwas, a research associate at the Cornell Center for       Astrophysics and Planetary Sciences (CCAPS) and the paper's second author.              The team estimated the companion galaxy, which they labeled SPT0418-SE,       was within 5 kiloparsecs of SPT0418-47, one of the brightest dusty,       star-forming galaxies in the early universe, its distant light bent       and magnified by a foreground galaxy's gravity into a circle, called an       Einstein ring. The Magellanic Clouds, satellites of the Milky Way are       about 50 kiloparsecs away.              The proximity suggests these galaxies are bound to interact with each       other and potentially even merge, an observation that adds to the       understanding of how early galaxies may have evolved into larger ones.              The two galaxies are modest in mass as galaxies in the early universe go,       with "SE" relatively smaller and less dusty, making it appear bluer than       the extremely dust-obscured ring. Based on images of nearby galaxies       with similar colors, the researchers suggest that they may reside       "in a massive dark-matter halo with yet-to-be-discovered neighbors."       Most surprising about the companion galaxy, considering its age and mass,       was its mature metallicity -- amounts of elements heavier than helium       and hydrogen, such as carbon, oxygen and nitrogen. The team estimated       that as comparable to our sun, which is more than 4 billion years old       and inherited most of its metals from previous generations of stars that       had 8 billion years to build them up.              "We are seeing the leftovers of at least a couple of generations of       stars having lived and died within the first billion years of the       universe's existence, which is not what we typically see," Vishwas       said. "We speculate that the process of forming stars in these galaxies       must have been very efficient and started very early in the universe,       particularly to explain the measured abundance of nitrogen relative to       oxygen, as this ratio is a reliable measure of how many generations of       stars have lived and died."        * RELATED_TOPICS        o Space_&_Time        # Galaxies # Astrophysics # Stars # Astronomy # Cosmology        # Big_Bang # Solar_System # Nebulae        * RELATED_TERMS        o Spitzer_space_telescope o Andromeda_Galaxy o        Barred_spiral_galaxy o Milky_Way o Globular_cluster o Galaxy        o Planetary_nebula o Large-scale_structure_of_the_cosmos              ==========================================================================       Story Source: Materials provided by Cornell_University. Original written       by James Dean, courtesy of the Cornell Chronicle. Note: Content may be       edited for style and length.                     ==========================================================================       Journal Reference:        1. Bo Peng, Amit Vishwas, Gordon Stacey, Thomas Nikola, Cody Lamarche,        Christopher Rooney, Catie Ball, Carl Ferkinhoff, Henrik        Spoon. Discovery of a Dusty, Chemically Mature Companion to a z ~        4 Starburst Galaxy in JWST ERS Data. The Astrophysical Journal        Letters, 2023; 944 (2): L36 DOI: 10.3847/2041-8213/acb59c       ==========================================================================              Link to news story:       https://www.sciencedaily.com/releases/2023/02/230227161428.htm              --- up 10 hours, 50 minutes        * Origin: -=> Castle Rock BBS <=- Now Husky HPT Powered! 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