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Raman Research Institute study finds X-ray pulsar Centaurus X-3 accretes matter through an accretion disk, rare for high-mass binaries

Scientists of the Raman Research Institute (RRI), led by Kinjal Roy, found that the bright X-ray pulsar Centaurus X-3 draws in matter through an accretion disk, which is rare for high-mass X-ray binaries, as per a DST release of 21 October 2026.

Summary

Scientists from the Raman Research Institute (RRI), an autonomous institute of the Department of Science and Technology, found that Centaurus X-3, one of the brightest X-ray pulsars, accretes material through an accretion disk. Led by researcher Kinjal Roy, the team studied four secondary emission lines and traced their variation to an accretion stream that co-rotates with the pulsar, which can exist only if a disk is present. This is rare because high-mass X-ray binaries usually capture matter directly from the companion star's wind. Centaurus X-3, about 24,000 light years away, was one of the first X-ray pulsars discovered.

Key facts

Object
Centaurus X-3 (X-ray binary pulsar)
Type
High-mass X-ray binary (companion over 10 times Sun's mass)
Distance
About 24,000 light years, constellation Centaurus
Finding
Accretion through an accretion disk (rare for HMXBs)
Evidence
Variation in four secondary emission lines due to co-rotating accretion stream
Institute
Raman Research Institute (autonomous, DST)
Lead researcher
Kinjal Roy
Usual HMXB accretion
Direct capture of stellar wind

Practice MCQs 2 questions

Q1 Advanced

Scientists of which institute reported in October 2026 that the X-ray pulsar Centaurus X-3 accretes matter through an accretion disk?

Show answer

Correct answer: C — Raman Research Institute

PIB (DST): Scientists from the Raman Research Institute (RRI), an autonomous institution of DST, led by Kinjal Roy, made the finding.
Q2 Advanced

Why is the finding about Centaurus X-3 (October 2026) considered unusual?

Show answer

Correct answer: D — High-mass X-ray binaries usually accrete by directly capturing stellar wind, not through an accretion disk

PIB (DST): Accretion in this system occurs through an accretion disk, which is rare in high-mass binaries; in HMXBs accretion generally happens through direct capture of stellar wind.

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