The Hubble Space Telescope has discovered white dwarfs that burn hydrogen on their surface, slowing down their cooling rate. This finding challenges the conventional view of white dwarfs as inert, slowly cooling stars.
An international team has identified five objects that could help distinguish brown dwarfs from low-mass stars. The companions, characterized by periods of 5-27 days and radii between Jupiter's, provide valuable information about their composition and formation.
New research reveals that magnetic fields of middle-aged stars become sub-critical, leading to reduced angular momentum losses and altered magnetic field strengths. This phenomenon breaks the relationship between a star's age and its rotation rate, allowing for a diversity of solar-stellar phenomena.
New models of neutron stars show mountains only a fraction of millimetres high, contradicting previous estimates. The research used computational modelling to study the role of ultra-dense nuclear matter in supporting these tiny mountains.
Researchers confirmed detection of two rare events involving collision of black hole and neutron star, producing strong gravitational waves signals. The mergers involved massive objects with masses up to 9 solar masses and 1.9-solar-mass neutron stars, providing new information on binary systems and their properties.
Researchers have detected two events of black holes merging with neutron stars, providing insights into their origins and merger rates. The findings will enable the drawing of conclusions about the host of astrophysical models of compact object formation and binary evolution.
Astronomers using Gemini Observatory and WIYN 3.5-meter Telescope found 73 binary star systems among TESS exoplanet hosts, which could be hiding Earth-sized planets. The team discovered that small planets are harder to detect in binary systems due to glare from the companion star.
Researchers used Gaia eDR3 catalog data to determine which stars pass through the Earth Transit Zone over a 10,000-year period. This allows nearby star-systems to potentially detect Earth, with 1,715 systems having had this opportunity since human civilization began.
The Milky Way's galactic bar has slowed down its spin by at least 24% since its formation, according to a study published in Monthly Notices of the Royal Astronomical Society. Dark matter acts as a counterweight slowing the spin.
Satellite galaxies that orbit massive central galaxies can form new stars due to active black holes clearing their path through intergalactic gas. Researchers used systematic observations and cosmological simulations to find this counter-intuitive effect.
A team of astrophysicists led by Luke Bouma has confirmed that one of these streams of stars, NGC 2516, extends at least 1,600 light-years -- 500 parsecs -- from tip to tip.
Astronomers have discovered a massive open cluster of intermediate age in the Scutum constellation, containing at least 15,000 stars. The Valparaíso 1 cluster was detected using Gaia satellite data and is notable for its unexpected discovery in a well-explored part of the sky.
A team of scientists discovered that three dozen dwarf galaxies simultaneously accelerated their star birth rates, defying expectations. The galaxies, separated by up to 13 million light-years, had a synchronized decrease in stellar birth rate 6 billion years ago and an increase 3 billion years ago.
Astronomers will use the James Webb Space Telescope to study a region of gas and dust in the Orion Nebula called the Orion Bar, which is shaped by intense ultraviolet light from young stars. The team hopes to understand how massive stars influence their environments and even the formation of our own solar system.
Using new methods in astronomy, researchers have identified the most precise ages of red giant stars in the galaxy, shedding light on the timing of the early Milky Way's formation. The study suggests that the merger with the satellite galaxy Gaia-Enceladus occurred around 10 billion years ago.
Researchers have dated the oldest stars in our galaxy with unprecedented precision by combining data from their oscillations with information about their chemical composition. The team found that these ancient stars were originally part of a satellite galaxy called Gaia-Enceladus, which collided with the Milky Way early in its history.
A team of astronomers has measured internal mixing within an ensemble of massive stars using observations of stellar oscillations. The results show that the mixing is diverse, unrelated to star mass or age, and influenced by internal rotation. This study provides new insights into the evolution and structure of massive stars.
Researchers used asteroseismology to measure the spin of older stars, finding they rotate faster than predicted by magnetic braking theories. The study provides new insights into the weakening effects of magnetic braking on older stars.
A survey of star formation in the Orion Nebula Cluster found similar mass distributions for newborn stars and dense gas cores, suggesting that gas accretion rate determines final star mass. The results contradict the core-collapse model, supporting the competitive accretion model instead.
Researchers identify five double star systems, Kepler-34, -35, -38, -64 and -413, as potential candidates for supporting life. The study shows that these systems have a permanent Habitable Zone, where liquid water could persist on the surface of any Earth-like planets.
Researchers found that neural networks trained on sound files of human language reached higher performance in image recognition, identifying objects and animals correctly 92% of the time. Using sound as a training tool improved results even with limited training data, outperforming traditional binary input methods.
Researchers at the University of Bath used resonance in spiraling neutron stars to measure symmetry energy, a key property of nuclear matter. This discovery sheds light on the fundamental workings of nuclei and offers insights into the forces that bind sub-atomic particles.
Astronomers discovered over 800 dense gas and dust cores near the Galactic Center, which may be 'stellar eggs' hatching into baby stars despite harsh conditions. The findings suggest that star formation is more resilient than thought, with ALMA observations detecting small outflows indicative of star birth.
Astronomers have studied the rare RV Tauri variable U Monocerotis, a binary system with two stars orbiting within a sprawling disk of dust. The 130-year dataset reveals predictable brightness changes and X-ray emissions.
Research from Binghamton University found that star employees take most of the credit for successful collaborations and most of the blame for failed ones, affecting non-star collaborators' careers. Non-stars may benefit from working with stars despite not receiving equal rewards or penalties.
A new theory, MeshCODE, proposes that memories are written in the shape of molecules in synaptic scaffolds, forming a complex binary code. This discovery may lead to a new understanding of brain function and treating brain diseases like Alzheimer's.
Astronomers have created a massive atlas of widely separated binary stars within 3,000 light years of Earth, comprising 1.3 million pairs. This increase in sample size provides insights into the evolutionary phases of these binaries, including 17,000 white dwarfs.
A new study using the Very Long Baseline Array (VLBA) has refined the distance to Cygnus X-1 and found its black hole mass to be approximately 21 solar masses, exceeding current stellar evolution models. This massive black hole suggests that lower mass loss through stellar winds during progenitor star evolution may have occurred.
Astronomers used Hubble and Gaia data to analyze the positions and velocities of stars in NGC 6397, finding strong evidence for invisible mass in the dense central regions. The bulk of this unseen mass is likely made up of stellar-mass black holes, rather than white dwarfs or neutron stars.
University of Warwick astronomers detect lithium and potassium in the atmospheres of four nearby white dwarf stars, revealing remnants of rocky planet crusts. The chemical composition of these crusts is similar to Earth's continental crust, providing a glimpse of the planets that may have orbited these dying stars billions of years ago.
Researchers have mapped the orbit of a rare Nitrogen-rich Wolf-Rayet star in the WR 133 binary system, marking the first-ever visually observed orbit of this type. The team determined the dynamical mass of both stars, with the WN star having 9.3 times more mass than our Sun.
Research reveals that galaxies with larger, 'puffy' disks continue to form stars over a longer period after cosmic noon. This is due to the cooler gas and lower influence of black holes, allowing for continued star formation. By studying galaxy disk size, astronomers can now accurately predict when star formation will cease.
Researchers discovered that the two stars in the HS Hydrae system were almost completely eclipsing each other 50 years ago but now barely overlap. The team predicts that the eclipses will cease around February 2021, marking the end of this rare stellar dance.
Astronomers using ALMA have observed a distant galaxy losing its ability to form stars after ejecting nearly half of its star-forming gas. The galaxy's gas ejection is happening at an alarming rate, equivalent to 10,000 Suns-worth per year.
Researchers used combined signals from binary neutron star mergers to study ultra-dense matter and constrain the Hubble constant. The analysis, led by Tim Dietrich, provided new insights into neutron star equation of state and expansion rate of the Universe.
Researchers have discovered a binary system of brown dwarfs, orbiting each other at an unprecedented distance, with one object being similar in mass to Jupiter and the other about 8 times less massive. This rare find suggests that star formation processes can create binary systems like those found in our solar system on smaller scales.
The new data includes exceptionally accurate measurements of the 300,000 stars within the closest 326 light years to the Sun. Researchers predict how the star background will change in the next 1.6 million years and confirm that the Solar system is accelerating in its orbit around the Galaxy.
A team of researchers has analyzed data to infer the nature of compact object orbiting within LS 5039, the brightest gamma-ray binary system in the Galaxy. The team suggests that particle acceleration process is caused by interactions between dense stellar winds and ultra-strong magnetic fields of a rotating magnetar.
A team of scientists has detected neutrinos from the sun directly revealing that the carbon-nitrogen-oxygen (CNO) fusion-cycle is at work in our sun. This detection confirms the CNO cycle as the dominant energy source powering stars heavier than the sun.
The team observed the nebula with two different spectrographs on large telescopes, finding that the central star is inflated and signatures of accretion are present. The data suggest a merging binary star system, offering a clear view of the central stellar remnant.
A study of ancient star orbits reveals unexpected patterns, contradicting previous assumptions about the Galaxy's metal-poor stars. The research, conducted by a team of astronomers, found that some of these stars orbit in previously unpredicted paths, similar to the Sun's path within the disk.
The ULLYSES program aims to create a comprehensive dataset for understanding star formation and its impact on planet habitability. The Hubble Space Telescope will observe over 300 stars across eight regions, capturing their spectral templates to inform research on stellar evolution and planetary chemistry.
Researchers from the University of Michigan found that the vast majority of field massive stars in the Small Magellanic Cloud are 'runaways,' or stars ejected from clusters. They discovered that these stars could have formed in isolation or were dynamically ejected due to unstable orbital configurations.
A team of scientists has created the most detailed family portrait of black holes to date, analyzing gravitational-wave data from LIGO and Virgo detectors. The study reveals new clues about black hole formation and tests Einstein's theory of general relativity, passing all tests with flying colors.
For the first time, astronomers have surveyed over 250 million stars in the Milky Way's bulge, measuring their chemical composition and gaining new insights into the galaxy's formation. The data will help scientists understand how the Milky Way formed its central bulge and gain a better understanding of other galaxies.
Astronomers have found compelling evidence that planets start to form while infant stars are still growing. The ALMA radio observatory has captured a high-resolution image of the proto-star IRS 63 with multiple gaps and rings of dust, indicating that seeds of planets are forming in these cosmic cradles.
Researchers from the University of Texas at Austin and Georgia Tech used supercomputers to model the formation of the first stars, known as Population III or Pop III stars. Their simulations showed that these ancient stars forged heavier elements, such as carbon, which seeded the next generation of stars.
Researchers at Rensselaer Polytechnic Institute have discovered the first shell-like formations of stars in the Milky Way, created by a 2.7 billion-year-old broadside collision with a dwarf galaxy. The findings offer new insights into the ancient event and its potential implications for other stellar phenomena.
Astronomers at the University of Vienna used machine learning to trace groups of stars born together and found thousands of sibling stars surrounding well-known cores of star clusters. The discovery reveals that star clusters are enclosed in rich halos, or coronae, more than 10 times larger than previously thought.
A recent study from an international team led by Prof. ZHAO Gang, Prof. SHI Jianrong, and Dr. YAN Hongliang found that most lithium-rich stars are 'red clumps' rather than 'red giants'. The research provides new insights into the origin of the ancient element lithium.
A new study reveals the binary nature of a trans-Neptunian object, with two objects orbiting each other only 350 kilometers apart. The discovery was made possible by the Research and Education Collaborative Occultation Network (RECON), a citizen science project.
The team discovered two massive young stars shrouded by gaseous disks containing sodium chloride and heated water vapor. The disks are counter-rotating, indicating the pair may not be twins, but rather strangers formed in separate clouds.
Interactions with binary companions generate complex planetary nebula shapes by influencing the stellar wind of elderly stars. Leen Decin and colleagues observed AGB star winds using ALMA, finding none with spherical symmetry and instead distinct geometries similar to those in PNe.
A new analysis of galaxy evolution finds that neutron star collisions do not create the quantity of chemical elements previously assumed. Instead, an entirely different sort of stellar phenomenon - unusual supernovae with strong magnetic fields - is responsible for making most of the heavy elements, including gold.
Researchers found three large, misaligned dust rings around the young triple star system GW Ori, with sufficient dust for planet formation. A computer simulation suggests that a hidden planet may have carved out a dust gap and broken the disk at the location of the current inner and outer rings.
Two teams of astronomers used ALMA to discover a misaligned ring system in the planet-forming disk of GW Orionis, a triple star system. The findings suggest that either gravitational pull from the stars or a newborn planet caused the misalignment, highlighting the complex processes involved in planetary formation.
A team of astronomers identified the first direct evidence that groups of stars can tear apart their planet-forming discs, leaving them warped and with tilted rings. This discovery suggests exotic planets may form in inclined rings around multiple stars.
A team of experts identified a stellar system where planet formation might take place in inclined dust and gas rings within a warped circumstellar disc around multiple stars. The discovery reveals that the inner ring contains 30 Earth masses of dust, which could be enough to form planets.
Scientists successfully simulated the crushing pressure of white dwarf stars to describe matter behavior, particularly in areas with oscillations. The findings could lead to new approaches for creating novel materials in laboratories.
Researchers have found that dormant small galaxies can slowly accumulate gas over billions of years, allowing for the formation of new stars. The study's findings shed light on the mysterious process of star formation in dwarf galaxies, providing insights into astrophysical processes.