Globular Clusters tagged posts

An international team of astronomers has discovered the remnant of an ancient collection of stars that was torn apart by our own galaxy, the Milky Way, more than two billion years ago.

The extraordinary discovery of this shredded ‘globular cluster’ is surprising, as the stars in this galactic archaeological find have much lower quantities of heavier elements than in other such clusters...

Hubble Space Telescope image of the young massive star cluster R136 in the 30 Doradus star forming region in the Large Magellanic Cloud. The core of this cluster contains several very massive stars with masses of several 100 times the mass of the Sun, which could have formed by stellar collisions. Credit: NASA, ESA, and F. Paresce (INAF-IASF, Bologna, Italy), R. O’Connell (University of Virginia, Charlottesville), and the Wide Field Camera 3 Science Oversight Committee

A team of international astrophysicists may have found a solution to a problem that has perplexed scientists for more than 50 years: why are the stars in globular clusters made of material different to other stars found in the Milky Way? In a study published by Monthly Notices of the Royal Astronomical Society, the team led ...

This is a binary star evolution within a globular cluster. Credit: Mark A. Garlick/University of Warwick

Comprised of hundreds of thousands of stars densely packed into a tight ball, globular clusters had been thought to be almost as old as the Universe itself – but thanks to newly developed research models it has been shown that they could be as young as 9 billion years old rather than 13 billion.

The discovery brings into question current theories on how galaxies, including the Milky Way, were formed – with between 150-180 clusters thought to exist in the Milky Way alone – as globular clusters had previously been thought to be almost as old as the Universe itself.

Designed to reconsider the evolution of stars, the new Binary Population and Spectral Synthesis (BPASS) models take the detai...

Visualization of the gravitational wave emission from a pair of orbiting compact objects. Credit: NASA

Next-generation gravitational wave detector in space will complement LIGO on Earth. The historic first detection of gravitational waves from colliding black holes far outside our galaxy opened a new window to understanding the universe. A string of detections – 4 more binary black holes and a pair of neutron stars – soon followed the Sept. 14, 2015, observation. Now, another detector is being built. LISA is expected to be in space in 2034, and it will be sensitive to gravitational waves of a lower frequency than those detected by the Earth-bound Laser Interferometer Gravitational-Wave Observatory (LIGO).

A new Northwestern University study predicts dozens of binaries (pairs of orbiting co...