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Black holes are objects with a gravitational pull so strong that not even light can escape. They are the subjects of intense scrutiny from astronomers from all over the world. Scientists across the world are studying their formation.
One way of forging black holes is the deaths of massive stars in Gamma Ray Bursts explosions so powerful that they have been called mini big-bangs. They send intense jets of light and high-energy radiation shooting across the universe.
Another way to create Gamma-ray Bursts (GRBs) is the collision of two neutron stars the kind of events that generate gravitational waves. Astronomers study the Gamma-rays and X-rays from such bursts to better understand explosion and black hole formation.
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“One of these instruments is the Cadmium Zinc Telluride Imager (CZTI) – which has just witnessed the birth of a black hole for the five hundredth time, the Inter-University Centre for Astronomy and Astrophysics (IUCAA) said in a statement.
This is a landmark achievement,” said Prof Dipankar Bhattacharya of Ashoka University and IUCAA, who is the current Principal Investigator of CZTI.
The wealth of data obtained by CZTI on Gamma Ray Bursts is making a big impact worldwide, he added.
CZTI has been studying GRBs since it first opened its eyes 6.5 years ago. The very first scientific result from AstroSat was the detection of GRB 151006A: just hours after the instrument was powered on after launch, said Prof. Varun Bhalerao, who leads the GRB search effort.
A unique aspect of CZTI is the ability to measure the polarisation of X-rays: an ability that is lacking in flagship missions like NASA’s Neil Gehrels Swift Telescope or the US-Europe Fermi Space Telescope.
Tanmoy Chattopadhyay, of the US-based Stanford University, has played a key role in these polarisation studies.
Polarisation tells us what is happening just outside the newly formed black hole. It is the most important measurement to distinguish between different theories of Gamma-ray Bursts, said Chattopadhyay.