As we gaze into the night sky from a remote and dark location, we are captivated by the multitude of stars that expand across the sky. In such pristine conditions, attempting to enumerate the exact quantity of stars visible to the naked eye becomes almost impossible. Despite the overwhelming number of stars, a common perception arises: that each star resides in solitary within the remote corners of our Universe. This notion appears reasonable given the colossal scale of the sky; stars seem to occupy their own cosmic niches without apparent interaction.
However, the reality is quite different. Many stars do not exist in isolation; instead, they engage in dynamic relationships within binaries, clusters, and association systems. Far from being solitary entities, a significant proportion of stars are accompanied by other celestial objects, interacting altogether. These systems, commonly termed star systems, showcase the rich tapestry of interstellar connections that punctuates the vastness of the universe.
What can we learn from star systems?
Stars like company. They can form binary systems, where two stars orbit each, but can also exist in more complex configurations consisting of three or more stars. The study of these stellar systems, whether in binary pairs or more complex systems, enhances our understanding of star formation and evolution.
Star Formation: The exploration of multiple star systems has significantly advanced our understanding of their formation pathways. The discovery of binary star and compact triple systems, for example, has revealed that they often form through disk fragmentation followed by gas accretion-driven inward migration. In contrast, higher-
order systems seem to primarily form through inside-out processes, where the inner parts of the stars take shape first.
Star Evolution: The wealth of information derived from studying star systems has also highlighted the role of binary systems as fundamental building blocks for comprehending the evolution of higher-order systems. Close binary systems, where stars are in proximity (within approximately less than 10 astronomical units), offer insights into the underlying physics behind of mass and angular momentum transfer and loss between stars. These processes can lead to the formation of chemically unique stars, characterised by enhancements in carbon and heavy elements. Examples include Barium stars (where there’s an overabundance of ionised Ba), CH starts (with strong spectral absorption bands due to the methylidyne radical CH), and carbon-enhanced metal-poor stars.
This knowledge extends beyond merely describing the chemical composition of stars; it also allows us to interpret various astronomical observations resulting from past merger events in higher-order stellar systems. Examples include phenomena like the Betelgeuse cloud high spin, the 19th-century supernova impostor event of Eta Carinae, and even the generation of gravitational waves—all of which could be attributed to merging events within high-order star systems.
Astronomical surveys
Observational astronomy is ushering in a new era for space exploration, driven by our rapid technological progress. The continuous refinement of telescopes, coupled with the integration of machine learning algorithms into data processing pipelines, exemplifies the cutting-edge tools that are propelling our exploration of the cosmos.
Among the ground-breaking initiatives driving this progress are sky surveys, which afford us unprecedented insights into the universe (Figure 1). An astronomical sky survey constitutes a comprehensive map or image of a specific region of the sky. Most surveys have focused on detecting exoplanets and studying the history and formation of the Milky Way. However, these same surveys have also played a pivotal role in allowing systematic searches for binary and higher-order star systems throughout the cosmos.