Near the centre of the Milky Way, a swarm of stars hurtles around a supermassive black hole at extraordinary speeds. Studying them could be the key to understanding our galaxy
Combining cold dark matter simulations with observations of stellar streams and globular clusters, researchers inferred a declining power-law initial mass function for globular clusters.
New research explains why globular clusters possess far fewer binary stars than the solar neighborhood. The study identifies 'black hole burning' within dense cluster cores as the primary driving mechanism.
Researchers identified a new globular cluster, HSC 61, belonging to the Sagittarius dwarf galaxy. The study mapped its stellar stream, determined its metallicity, and analyzed the Sagittarius merger event.
NASA, Hubble uzay teleskobunun yakaladığı ilginç bir kareyi paylaştı. Kameraya gülümseyen bir galaksi kümesi... ABD Havacılık ve Uzay Ajansı'nın (NASA) Hubble uzay teleskobu, evrenin gizemlerini gözlemlemeyi sürdürüyor. NASA 1990 yılından bu yana yörüngede çalışan Hubbe'ın kaydettiği çarpıcı bir…
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