Science & Tech

ISRO Scientists Detect Emissions From Black Hole

The radiation is being emitted by the black hole, Large Magellanic Cloud X-3 (LMC X3), a binary star system consisting of a black hole and larger than the Sun.
Sputnik
Scientists from the Indian Space Research Organisation (ISRO) and India's premier institute, the Indian Institute of Technology (IIT), have detected polarised emissions from a black hole source using the X-ray polarimetry technique.
The Scientists investigated the X-ray polarization properties of LMC X3, considered an ideal cosmic laboratory to study the X-ray polarization signatures, using Imaging X-ray Polarimetry Explorer (IXPE).
Polarised emissions may arise from the combined effects of direct and reflected emissions from a partially ionised disk atmosphere, the scientists concluded.

"Intense gravitational fields can cause the emitted light from black holes to become polarized. Our observations indicate that LMC X3 likely harbours a black hole with low rotation rate, surrounded by a slim disc structure that gives rise to the polarized emissions," wrote Dr Anuj Nandi, scientist about the study, which is now published at Monthly Notices of the Royal Astronomical Society.

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