. | . |
Astronomers find young galaxy with record-low oxygen levels by Brooks Hays Washington DC (UPI) Aug 03, 2020 Astronomers have discovered a tiny, young, metal-poor galaxy with the lowest oxygen abundance ever recorded. To find the tiny galaxy, researchers used machine learning algorithms to parse data collected by a pair of telescopes in Hawaii, the Subaru Telescope and W. M. Keck Observatory. Most galaxies in the modern universe are fairly large and mature, but models suggest there are still a handful of star-forming regions hiding among the masses of mostly dormant galaxies. Predicting their existence is one thing, but finding tiny, star-producing galaxies is another, researchers say. "To find these very faint, rare galaxies, deep, wide-field imaging data taken with the Subaru Telescope was indispensable," lead researcher Takashi Kojima, astronomer at the University of Tokyo Institute for Cosmic Ray Research, said in a news release. Subaru's wide-field survey has revealed 40 million objects. To process such a large set of data, researchers trained a machine learning algorithm to search for the type of spectroscopic signature -- the unique combination of light frequencies -- produced by early stages of galaxy formation. The algorithm identified 27 candidates. Scientists used the Keck Observatory's DEep Imaging and Multi-Object Spectrograph, or DEIMOS, as well as Subaru Telescope's Faint Object Camera and Spectrograph, to study each candidate. The follow-up observations revealed one of the candidates, HSC J1631+4426, to be extremely metal-poor and with record low levels of oxygen. Scientists described their discovery Monday in the Astrophysical Journal. An early version of their paper was published online at arxiv. "What's surprising is the stellar mass of the HSC J1631+4426 galaxy is very small, 0.8 million solar masses, which is only about 1/100,000 of our Milky Way, and comparable to the mass of a star cluster in our galaxy," said study co-author Masami Ouchi, a professor at the National Astronomical Observatory of Japan and the University of Tokyo. Researchers suggest low-mass, young, metal-poor galaxies like HSC J1631+4426 can help cosmologists better understand the evolution of galaxies shortly after the Big Bang, when the cosmos was just a few hundred million years old. Because the Big Bang generated large amounts of hydrogen and helium, oxygen was in relatively short supply among the earliest galaxies. Astronomers suggest HSC J1631+4426 might be more than just rare-- it may mark the end of a cosmic epoch. Models suggest that as the universe expands, matter will become too sparse to birth new galaxies, so HSC J1631+4426 could be the last of its kind, researchers say.
Astrophysicists Observe Long-Theorized Quantum Phenomena Baltimore MD (SPX) Aug 03, 2020 At the heart of every white dwarf star - the dense stellar object that remains after a star has burned away its fuel reserve of gases as it nears the end of its life cycle - lies a quantum conundrum: as white dwarfs add mass, they shrink in size, until they become so small and tightly compacted that they cannot sustain themselves, collapsing into a neutron star. This puzzling relationship between a white dwarf's mass and size - called the mass-radius relation - was first theorized by Nobel Prize-w ... read more
|
|
The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us. |