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Picture: Hubble Examines a Dwelling Place for Aging Stars

This photograph, captured by the NASA/ESA Hubble Space Telescope’s Wide Field Planetary Camera 2, displays the globular cluster Terzan 1. Situated approximately 20,000 light-years away from us in the Scorpius constellation, it is one of the 150 globular clusters that belong to our galaxy, the Milky Way.Typical globular clusters consist of roughly a hundred thousand stars, bound together by their mutual gravitational attraction, forming a spherical shape spanning a few hundred light-years. It is believed that every galaxy possesses a population of globular clusters. While the Milky Way has a few hundred, giant elliptical galaxies can have several thousand.

These clusters house some of the oldest stars within a galaxy, which explains the reddish hues of the stars in this image. The bright blue stars, on the other hand, are foreground stars and not part of the cluster. The ages of the stars in the globular cluster provide valuable insights into the early stages of galaxy formation. By studying them, we can enhance our understanding of how galaxies came into existence.Similar to many other globular clusters, Terzan 1 emits X-rays. It is likely that these X-rays originate from binary star systems that consist of a dense neutron star and a regular star. The neutron star accretes material from its companion star, resulting in a burst of X-ray emission. Subsequently, the system enters a quiescent phase during which the neutron star cools down and emits X-rays with distinct characteristics. Eventually, enough material accumulates from the companion star, triggering another outburst.

This image, taken with the Wide Field Planetary Camera 2 on board the NASA/ESA Hubble Space Telescope, shows the globular cluster Terzan 1. Lying around 20 000 light-years from us in the constellation of Scorpius (The Scorpion), it is one of about 150 globular clusters belonging to our galaxy, the Milky Way. Typical globular clusters are collections of around a hundred thousand stars, held together by their mutual gravitational attraction in a spherical shape a few hundred light-years across. It is thought that every galaxy has a population of globular clusters. Some, like the Milky Way, have a few hundred, while giant elliptical galaxies can have several thousand. They contain some of the oldest stars in a galaxy, hence the reddish colours of the stars in this image — the bright blue ones are foreground stars, not part of the cluster. The ages of the stars in the globular cluster tell us that they were formed during the early stages of galaxy formation! Studying them can also help us to understand how galaxies formed. Terzan 1, like many globular clusters, is a source of X-rays. It is likely that these X-rays come from binary star systems that contain a dense neutron star and a normal star. The neutron star drags material from the companion star, causing a burst of X-ray emission. The system then enters a quiescent phase in which the neutron star cools, giving off X-ray emission with different characteristics, before enough material from the companion builds up to trigger another outburst.

This article is republished from PhysORG under a Creative Commons license. Read the original article.

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