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Indian researchers discover ultra-compact stellar binary system with rare brown dwarf companion

Artistic impression of the discovered compact binary system showing a BSS primary orbited by a BD companion in an ultra-short, nearly circular orbit with a period of about 5.6 hours

A team of Indian and international researchers has discovered one of the shortest-period stellar binary systems known so far, featuring a blue straggler star paired with a rare brown dwarf companion in an ultra-compact orbit.

The discovery, announced by the Ministry of Science and Technology on Tuesday, is being seen as a significant breakthrough in understanding stellar evolution and the formation of exotic binary systems.

The study, published in the journal Monthly Notices of the Royal Astronomical Society: Letters, confirms the first known case of a blue straggler star hosting a substellar brown dwarf companion in a compact binary system.

Blue straggler stars have long puzzled astronomers because they appear brighter and bluer than other stars of similar age in star clusters, seemingly defying standard models of stellar evolution.

The research was carried out by scientists from Gauhati University, the Indian Institute of Astrophysics, Aryabhatta Research Institute of Observational Sciences and the INAF-Catania Astrophysical Observatory.

The team found that the binary system has an exceptionally short orbital period of around 5.6 hours, or 0.234 days, making it one of the most compact systems of its kind discovered to date.

Researchers said the companion object has a mass of nearly 0.056 times that of the Sun, placing it below the hydrogen-burning limit and firmly in the category of brown dwarfs — celestial objects too massive to be planets but too small to sustain nuclear fusion like stars.

According to the researchers, the system lies within the so-called “brown dwarf desert”, a region where such companions are considered extremely rare. The study describes it as the shortest-period binary system discovered in this category.

The team included researchers Ali Hasan Sheikh and Prof. Biman J. Medhi from Gauhati University, Dr. Sergio Messina from the INAF-Catania Astrophysical Observatory, Prof. Annapurni Subramanium and Prof. Ram Sagar from the Indian Institute of Astrophysics, and Dr. Neelam Panwar from ARIES, Nainital.

Scientists believe the system may have formed through the evolution of a hierarchical triple-star system, involving mass transfer, orbital interactions and eventual merger processes that resulted in the present compact binary configuration.

The researchers said the findings could help refine theoretical models related to stellar evolution, binary star interactions and substellar objects, while also improving interpretation of observations from ground-based and space telescopes.

The study also highlights how archival astronomical data, combined with innovative analysis, can lead to major discoveries without requiring expensive new observational infrastructure.

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