NGC 3310 is forming clusters of new stars at a prodigious rate, with hundreds of individual young, luminous stars visible throughout the galaxy. The wide range of cluster ages suggests that the starbursting can continue for an extended interval, once triggered.
A team of Belgian and French astronomers have discovered three distant stars with extremely high Lead abundances, exceeding other elements heavier than Iron. This finding aligns with current stellar models predicting the buildup of heavy elements in stellar interiors.
Research suggests that brown dwarfs don't require special conditions to form, but rather are ejected from multiple-star systems due to gravitational interactions. This process affects their growth and ultimately determines their fate as either a normal star or a brown dwarf.
Astronomers have discovered over 154 rapidly moving stars towards the center of the Milky Way and its brightest neighboring galaxy. The findings are significant as these stars were previously difficult to detect due to their extreme density, allowing scientists to gain insights into the galaxy's most densely packed regions.
A team of astronomers, including an undergraduate researcher, detect the presence of massive stellar explosions in a distant galaxy using quasar light. The discovery reveals six super bubbles formed at nearly the same time, releasing energy equivalent to 10,000 suns over their lifetimes.
Researchers identified 168 young stars in the Orion star forming complex, about half the mass of the sun. The discovery provides important constraints for theories on how fast planetary systems can form, suggesting solar-like stars can form planets in around 10 million years.
Astronomers using Chandra X-ray Observatory have discovered that protostars, the youngest stage of star formation, are marked by powerful X-rays from plasma ten times hotter and 100 to 100,000 times brighter than our Sun's flares. This has provided the closest look yet at the youngest stars in the Universe.
The W49 cluster is believed to contain approximately 100 type O stars, the hottest and most massive stars in our galaxy, all less than 1 million years old. This young star cluster is part of a larger birthing process that will eventually lead to globular clusters like those orbiting the Milky Way.
Researchers using the VLA radio telescope found a pulsar that is at least 40,000 years old and may be as old as 170,000 years. This discovery challenges current understanding of neutron stars and their ages.
Astronomers have directly detected a new type of stellar flare on the binary system HR 1099, challenging current models and providing insight into flare physics. The flares were observed in a narrow temperature range of gas on the star, distinct from the hot gas that emits X-rays.
A new study published in the journal Science suggests that low-mass stars called red supergiants may die explosively rather than fade away quietly. This discovery has significant implications for our understanding of nucleosynthesis, stellar structure, and the evolution of stars.
The discovery sheds light on the formation and death of stars, revealing intricate structures such as neutron stars, black holes, and X-ray binary systems. The image provides valuable insights into the distribution of heavy atoms throughout the universe, offering a glimpse into the early history of the cosmos.
NASA's Chandra X-ray Observatory has detected nearly a thousand faint X-ray-emitting stars in the young star-forming region of the Orion Nebula. The discovery will help unravel the astrophysical principles underlying violent magnetic activity in young stars.
A Yale researcher has discovered up to 70 new and very distant RR Lyrae stars in the Milky Way that can provide valuable clues about the galaxy's history and composition. The stars are thought to be among the oldest in the galaxy, with ages of over 12 billion years.
Six new planets have been discovered orbiting nearby stars, bringing the total number of known planets outside our solar system to 28. The newly discovered planets are located within the habitable zones of their stars and have temperatures suitable for liquid water to exist in one case.
When a star swallows a planet, it can experience profound effects on its evolution, including changes in spin rate and emission of infrared radiation. The simulations show that large planets can survive for thousands of years before being vaporized by the heat, leaving behind tell-tale signs such as high lithium abundance.
Researchers have found two nearby streams of stars that appear to be debris from a single dwarf galaxy torn apart by the Milky Way's gravity about 10 billion years ago. These relic streams are part of the Milky Way's outer structure and provide insights into its formation.
Dr. Karen Kwitter's research focuses on the chemical composition of planetary nebulae, which can reveal information about the life cycle of stars and the evolution of our galaxy. By analyzing light spectra from these clouds, she aims to refine models of galactic chemical evolution.
Guillermo Gonzalez argues that the Sun's exceptional characteristics made intelligent life emerge on Earth. The Sun is unusually massive and has a stable light output, making it an ideal place for life to thrive. This rules out over 95% of stars in the Galaxy as potential candidates.
A team of astronomers has discovered a unique cluster of young stars, approximately 8 million years old, located 97 parsecs from Earth. The cluster, centered around eta Chamaeleon, is one of the nearest to our planet and exhibits unusual characteristics.
A new Hubble image captures the entire stellar life cycle in a single photograph, showcasing various stages of star formation and evolution. The galaxy NGC 3603 is home to multiple starburst clusters, young massive stars, and a blue supergiant nearing its supernova fate.
An Australian-led team of astronomers has discovered a significant number of stray stars, potentially altering our understanding of the universe's composition. These findings suggest that there may be as many stars living in intergalactic space as those within galaxy clusters.
Astronomers have obtained the clearest view yet of the center of the Andromeda galaxy, revealing a double nucleus that has long puzzled scientists. The study uses new Hubble images to map the orbital motions of stars around the black hole at the galaxy's core.
Physicists suggest MACHOs may be made of a weird kind of mirror matter generated in the big bang, with potential for mirror planets and organisms. This theory could explain the presence of invisible stars on the outskirts of our Galaxy.
Detailed studies of 12 stars with Jupiter-mass planets show concentrations of heavy elements two to three times greater than in the sun. The discovery supports the theory that stars born in heavy-element-enriched clouds are more likely to harbor giant planets.
Astronomers have discovered a large number of slow X-ray pulsars in supernova remnants, which are believed to be neutron stars with huge magnetic fields. These so-called magnetars rotate much slower than expected and are invisible to radio probes.
Astronomers have discovered large numbers of previously unknown stars in the Virgo Cluster using dying green stars as tools. The findings suggest that at least 22% of Virgo's light is coming from these hidden stars, and could affect estimates of universe mass.
A team of astronomers led by Bo Reipurth and John Bally observed that ultraviolet radiation from nearby massive stars destroyed the cocoons of gas and dust surrounding young stars, revealing billions of miles long supersonic jets. The destruction has provided new insight into star birth and evolution, and may have implications for the ...
Researchers using Hubble Space Telescope spot large dust particles in rings around three stars, suggesting planets may be forming. The observations reveal a critical early stage in planetary evolution, with the potential for millions of years of dust grain aggregation to form planets.
A researcher has detected an enormous black hole at the center of the Milky Way galaxy, with a mass 2.6 million times that of our Sun. The discovery was made using advanced imaging techniques and provides a definitive view of a part of the galaxy previously unseen.
A new study published in the Astrophysical Journal Letters finds that a review of thousands of nearby stars failed to show any rogue stars capable of altering comet orbits and sending them towards Earth. The researchers used the HIPPARCOS catalogue, which measures the location and motion of over 120,000 stars, and found no evidence of a
A rapidly spinning neutron star, SAX J1808.4-3658, is providing proof for the theory that millisecond pulsars are propelled to mind-boggling speeds by accretion of material from a companion star. This discovery fills an important niche in our understanding of star evolution.
Astronomers have discovered expanding gas clouds thrown off by nuclear eruptions in stars, which provide reliable distances to these stars. The Hubble Space Telescope has captured detailed images of two nova shells, revealing structure and asymmetry, including polar blobs and equatorial rings.
Cornell University astronomers James Cordes and Barney Rickett have developed a method to calculate the speed and distance of extremely fast-moving neutron stars, called pulsars, by analyzing their twinkling rate. By combining data from two large radio telescopes, they can identify new pulsars and better understand their physics.
Astrophysicists have discovered rapid oscillations in neutron star brightness, which may confirm a unique effect of curved space-time predicted by Einstein's theory. The data was obtained using NASA's Rossi X-Ray Timing Explorer satellite.
Researchers outline three unique features that may distinguish strange stars from neutron stars, including higher X-ray energy and pulse emissions. The discovery of a strange star could prove the existence of quark matter, a form of matter made up of quarks.
Astronomers use Hubble Space Telescope images and a computer model to study the behavior of stars in their infancy, shedding light on how cosmic dust influences the environment. The findings provide new insights into the formation of solar systems and the role of powerful jets of dust and gas in shaping star formation.
Researchers from UD and Denmark confirmed Subramanyan Chandresekhar's theory on the structure of compact stars, including pulsars, black holes, and white dwarf stars. By analyzing distances to a dozen white dwarf stars using HIPPARCOS data, they verified the theory, which predicts the size of white dwarf stars based on their mass.
Researchers have detected unusual light patterns from faint stars in a globular cluster, suggesting catastrophic star interactions. The study's findings reveal that these clusters are regions of intense stellar activity, with stars locked in orbital duets that can prevent core collapse into black holes.
Researchers calculate neutron star's mass by measuring X-ray pulses from innermost orbit, revealing a massive star about twice the sun's mass. The findings provide new insights into the birth and evolution of neutron stars.