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
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
Space & AstronomyAstronomy#Chinese Academy of Sciences#Research News#astronomy#astrophysics
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
Space & AstronomyParticle PhysicsAstronomy#Chinese Academy of Sciences#Research News#astronomy#Space Exploration#astrophysics#Particle Physics#High Energy Physics
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
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
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 an important process in the evolution of the universe, often causing supermassive black holes in the centers of galaxies to approach each other. Triple galaxy merger events are relatively rare in the universe and provide a unique sample for studying the co-evolution of galaxies and black holes.
Space & Astronomy#Chinese Academy of Sciences#科研进展#CAS#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
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
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.
Space & Astronomy#University of Michigan#News Releases#Science & Technology#astronomy#black hole#galaxy#Michigan News#astrophysics
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.
Space & Astronomy#University of Wisconsin-Milwaukee#UWM Report#research#Science & Technology#astronomy#astrophysics
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
Space & Astronomy#Lawrence Livermore National Laboratory#Academic Engagement#Engineering#Lasers and Optical S&T#Top Story#astronomy#astrophysics#NSF–DOE Vera C. Rubin Observatory
Space & AstronomyPacific Northwest National Laboratory
Stars are born in dense gas fiber structures inside molecular clouds. The processes of fiber fragmentation, collapse and material accretion are core research topics in the field of contemporary astrophysics. For a long time, there have been two mainstream theories in the academic community regarding the formation mechanism of fiber structures: supersonic turbulence-dominated and gravity-dominated. Due to the lack of systematic dynamic statistical research on subparsec (less than 1 parsec), the two major theoretical models have always been difficult to fully test.
Space & Astronomy#Chinese Academy of Sciences#科研进展#CAS#astronomy#astrophysics
Space & AstronomyUniversity of California, Riverside
Previously, the large-scale "warp structure" of the Milky Way has been widely confirmed and a basic model has been established. However, compared with the overall structure, finer-scale vertical undulation structures such as folds in the galaxy disk have long lacked systematic observation and quantitative research. Carbon monoxide (CO) molecular gas is an important probe for tracking the cold and dense medium of the Milky Way. However, limited by survey sensitivity and spatial coverage, there are still obvious uncertainties in the three-dimensional structure of the Milky Way's outer disk. Previous observations of related molecular gas fold structures were limited to the solar neighborhood, and it is unknown whether they exist in the outer disk of the Milky Way.
Space & Astronomy#Chinese Academy of Sciences#科研进展#CAS#astronomy#astrophysics
