An international research team led by scientists from the Chinese Academy of Sciences (CAS) has discovered an isolated pulsar located within the tidal tail of NGC 6791, one of the oldest and most massive open clusters in the Milky Way. By combining observations from the Five-hundred-meter Aperture Spherical radio Telescope (FAST), the MeerKAT radio telescope and the Canada-France-Hawaii Telescope
Space & AstronomyAstronomy#Chinese Academy of Sciences#Research News#astronomy#astrophysics
In the vast cosmos, supernova explosions are widely regarded as the most brilliant fireworks in the universe. Among them, Type Ia supernovae (SNe Ia) are hailed as "standard candles" due to their highly consistent peak luminosity, making them a key tool for measuring cosmic distances. However, a recent study has found that even SNe Ia that appear nearly identical may hide small "genetic" differenc
Space & AstronomyAstronomy#Chinese Academy of Sciences#Research News#astronomy#astrophysics
Are the large-scale magnetic fields of magnetars dominated by a dipolar structure, or is a significant magnetic-field twist required to explain the observations? A recent study by researchers from the Xinjiang Astronomical Observatory (XAO) of the Chinese Academy of Sciences (CAS) has found that the observed X-ray polarization of two magnetars can be explained by dipole-dominated magnetic fields,
Space & AstronomyAstronomy#Chinese Academy of Sciences#Research News#astronomy#astrophysics
With a twist between layers of graphene, scientists supported by the DOE’s Office of Science created the foundation for twistronics.
FeaturesSpace & AstronomyTechnology & Innovation#DOE#Office of Science#astronomy#astrophysics#advanced materials#innovation#Oak Ridge National Laboratory#Lawrence Berkeley National Laboratory
The BESIII Collaboration, led by the Institute of High Energy Physics of the Chinese Academy of Sciences, has achieved the world's most precise measurement of the electric dipole moment (EDM) of the Lambda (Λ) hyperon using quantum-entangled Λ–anti-Λ pairs produced in J/ψ decays. The result improves the experimental sensitivity by about three orders of magnitude compared with the previous measurem
Space & AstronomyTechnology & InnovationParticle Physics#Chinese Academy of Sciences#Research News#Particle Physics#astronomy#astrophysics#advanced materials#innovation#Fermilab
Active galactic nuclei (AGN), powered by accreting supermassive black holes, and X-ray binaries (XRBs), powered by accreting neutron stars or stellar-mass black holes, are two representative classes of compact accreting systems. Relativistic collimated jets are among the most spectacular phenomena in these systems. Understanding how these powerful outflows are launched, accelerated, and collimated
Space & AstronomyAstronomy#Chinese Academy of Sciences#Research News#astronomy#astrophysics
The LUX-ZEPLIN experiment observed an unusual particle interaction, but researchers will need more data to confirm.
FeaturesSpace & AstronomyParticle Physics#DOE#Office of Science#astronomy#astrophysics#Particle Physics#High Energy Physics#Lawrence Berkeley National Laboratory
The universe has been having fewer and fewer stellar "babies". Over the past 4.5 billion years, the rate of star birth has crashed to less than half of what it once was. But here's the twist: the most essential "fuel" for making stars has barely decreased. This finding comes from an international team led by researchers from the Chinese Academy of Sciences (CAS), in collaboration with the Dark Ene
Space & AstronomyTelescopesSatellites#Chinese Academy of Sciences#Research News#Telescopes#Satellites#astronomy#astrophysics
Space & AstronomyWashington University in St. Louis
Ahead of the scheduled Aug. 30 launch of NASA’s Nancy Grace Roman Space Telescope, several Washington University in St. Louis researchers have been selected to play important roles in the mission’s inaugural science program. The Roman telescope promises to transform our understanding of the universe. NASA will use the Roman telescope to investigate dark energy, discover thousands of exoplanets and
Space & AstronomySpace#Washington University in St. Louis#Newsroom#astronomy#astrophysics
A research team from the Shanghai Astronomical Observatory (SHAO) of the Chinese Academy of Sciences (CAS) has discovered that satellite galaxies retain a measurable "kinematic memory" of matter flowing into and along cosmic filaments. Using a large spectroscopic sample from the Sloan Digital Sky Survey (SDSS) , the team found that satellite galaxies preferentially orbit within planes that contain
Space & AstronomyAstronomy#Chinese Academy of Sciences#Research News#astronomy#astrophysics
Thanks to significant philanthropic and foundation support over the last year, students across American University’s College of Arts and Sciences are turning what they learn into real-world impact.
Space & AstronomyEnvironment & ClimateResearch#American University#Research News#Research · August 20#research#astronomy#astrophysics#climate#decarbonization
Galaxy mergers are among the most spectacular and destructive events in the universe. During these encounters, not only are billions of stars redistributed, but the supermassive black holes lurking in the galaxies' centers can also interact with one another. Yet systems where three galaxies merge simultaneously are uncommon. Now, researchers have obtained the first direct observational evidence fo
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An international research team, including an astronomer from the University of Michigan, have revealed how certain black holes manage to eat and grow while simultaneously flinging their food across galaxies.
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Space & AstronomyUniversity of Wisconsin-Milwaukee
A few years ago, scientists discovered an unusual astronomical phenomenon: Objects that sent short bursts of radio waves at distinct intervals, emanating from various parts of space.
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The Large High Altitude Air Shower Observatory (LHAASO) revealed that the peculiar binary system Cygnus X-3 in the constellation Cygnus is the highest energy gamma-ray source known to date. The temporal variability and spectral characteristics measured by LHAASO confirmed this object as the source of cosmic rays, with particle energies reaching at least 30 PeV (1PeV=10 15 eV), far exceeding curren
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Space & AstronomyLawrence Livermore National Laboratory
The NSF-DOE Vera C. Rubin Observatory marked a major milestone with the beginning of the Legacy Survey of Space and Time (LSST), a 10-year effort to capture the universe in unprecedented detail. Lawrence Livermore National Laboratory (LLNL) engineer and former project manager for the LSST Camera, Vincent Riot reflected on the culmination of the project and the journey ahead. Development of the world's largest digital camera began before Riot arrived at the Lab in 2003. For most of his career, he worked to build first-of-its kind optical components, including lenses that would later be
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Space & AstronomyPacific Northwest National Laboratory
Recently, a research team from the Shanghai Astronomical Observatory (SHAO) of the Chinese Academy of Sciences (CAS), in collaboration with Anhui Normal University, used orbital similarity criteria and numerical simulations to systematically screen known near-Earth asteroids. They identified multiple groups of potential asteroid pairs that may share a common origin and estimated their possible sep
Space & AstronomyAstronomy#Chinese Academy of Sciences#Research News#astronomy#astrophysics
Space & AstronomyUniversity of California, Riverside
Book cover with a man standing on a yellow kite in a blue sky According to a new book by Queen Mary University of London academic Dr S M A Moin , the answer lies not in technology itself, but in the human capacity for imagination, ethical judgement and moral courage. Published today (31 July), Leadership in the Imagination Age: Navigating Unprecedented Possibilities and Moral Challenges argues tha
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Researchers have recently carried out 18-26 GHz broadband spectral-line observations of the W33 giant molecular cloud. Using the German Effelsberg 100-meter radio telescope, they determined the physical and chemical properties of the dense clumps within it . The study, led by Associate Researcher Kadirya Tursun of the star formation and evolution group at the Xinjiang Astronomical Observatory of t
Space & AstronomyAstronomy#Chinese Academy of Sciences#Research News#astronomy#astrophysics
Massive stars form within cold, dense molecular clouds, where gas contracts under gravity and can readily fragment into numerous smaller cores. A new study has revealed how massive stars avoid excessive fragmentation of their surrounding material and obtain sufficient "fuel" to sustain their growth. Recently, MENG Dezhao, a PhD student in the star formation and evolution group at the Xinjiang Astr
Space & AstronomyAstronomy#Chinese Academy of Sciences#Research News#astronomy#astrophysics