Ultra-bright X-ray source awakens near a galaxy not so far away

Artist's impression of an ultra-luminous X-ray pulsar
Artist’s impression of an ultra-luminous X-ray pulsar.
NASA / JPL-Caltech

A new ultra-bright source of X-rays has awakened in between our galactic neighbours the Magellanic Clouds, after a 26-year slumber. This is the second-closest such object known to date, with a brightness greater than a million Suns. The discovery is published in the journal Monthly Notices of the Royal Astronomical Society.

The object, known as RX J0209.6-7427, was first detected during a 6-month long outburst in 1993. Though it was initially identified as a Be-type X-ray binary, its true nature remained a mystery as it lingered in a dormant state for the next 26 years, only flaring up again in November last year.

Now, a team of Indian scientists have used AstroSat, India’s first dedicated space observatory, to reveal the extreme nature of the source, and have detected broad-energy X-ray pulsations in the object for the first time. This classifies it as a type of object known as an ultra-luminous X-ray pulsar (ULXP).

The pulsar is located in the Magellanic Bridge, a stream of gas and stars linking the Magellanic Clouds. These are two of our nearest galactic companions, and some of the most distant objects visible to the naked eye. The new X-ray source is the second-closest ULXP known to date, after a 2018 discovery in our own Milky Way galaxy, and is only the eighth such object ever discovered.

Ultra-luminous X-ray sources are observable as single points in the sky, but with brightnesses comparable to entire galaxies. “The conventional theory is that in order to shine so brightly, ULXPs must be glowing accretion discs around black holes,” said Amar Deo Chandra, lead author on the new study. “However, recent discoveries of pulsations in these objects suggest that they may in fact have neutron stars at their heart.”

A neutron star is the remnant of a dead star which contains as much matter as our Sun, but is compressed into a tiny radius of as little as 10km – the size of a small city. The neutron star in this object is thought to be spinning as rapidly as 100 times per second, and emits pulses of energetic X-rays from its magnetic poles, leading to the new ‘X-ray pulsar’ classification.

The group of astronomers, from IISER Kolkata, IUCAA Pune and the Center for Excellence in Basic Sciences (UM-DAE CEBS) Mumbai, have also found that the pulsar may even be speeding up, setting off bright X-ray ‘fireworks’. This is thought to happen when the neutron star captures material from a companion star, injecting energy into the system and speeding up the rotation.

The scarcity of similar sources makes detecting and studying new ULXPs essential for X-ray astronomers seeking to understand the Universe.

“This is only the eighth ULXP detected so far, and the first one near the Magellanic Clouds,” Chandra adds. “It raises the interesting possibility that a significant fraction of ultra-luminous X-ray sources may really be neutron stars accreting at super Eddington rates, rather than black holes as previously thought.”


Media contacts

Dr Morgan Hollis
Royal Astronomical Society
Mob: +44 (0)7802 877 700

Dr Robert Massey
Royal Astronomical Society
Tel: +44 (0)20 7292 3979
Mob: +44 (0)7802 877 699


Science contacts

Mr Amar Deo Chandra
Center of Excellence in Space Sciences India
Indian Institute of Science Education and Research
Kolkata, India
Tel: +9 177 38 510 420

Dr Jayashree Roy
IUCAA Pune, India
Tel: +9 179 00 164 536


Images and captions

Artist's impression of an ultra-luminous X-ray pulsar
Artist’s impression of an ultra-luminous X-ray pulsar.
NASA / JPL-Caltech


The AstroSat satellite in a clean room before its integration with PSLV-C30, and an artist's impression of the AstroSat space observatory in orbit
AstroSat in a clean room before its integration with PSLV-C30 (top panels), and artist's impression of the AstroSat space observatory in orbit (bottom panel).
Indian Space Research Organisation (ISRO)


Further information

The new work appears in, “Study of Recent outburst in the Be/X-ray binary RX J0209.6-7427 with AstroSat: A new ultraluminous X-ray pulsar in the Magellanic Bridge?”, A.D. Chandra, J. Roy, P.C. Agrawal, M. Choudhury,, Monthly Notices of the Royal Astronomical Society (2020), in press (DOI: 10.1093/mnras/staa1041).

A copy of the paper is available from: https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/staa1041


Notes for editors

The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organises scientific meetings, publishes international research and review journals, recognises outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 4,400 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.

The RAS accepts papers for its journals based on the principle of peer review, in which fellow experts on the editorial boards accept the paper as worth considering. The Society issues press releases based on a similar principle, but the organisations and scientists concerned have overall responsibility for their content.

In 2020 the RAS is 200 years old. The Society is celebrating its bicentennial anniversary with a series of events around the UK, including public lectures, exhibitions, an organ recital, a pop-up planetarium, and the culmination of the RAS 200: Sky & Earth project.

Follow the RAS on Twitter, Facebook, Instagram and YouTube

Download the RAS Podcast from Audioboom


Submitted by Morgan Hollis on Mon, 01/06/2020 - 15:33