IISc researchers observed the black hole X-ray binary IGR J17091–3624 and studied the variations in its flickers to study whether they were truly random or just chaotic.

IIT Bombay study says high energy gravitational waves might be the instigator of FRBs

Dr. Harsh Vardhan, Hon’ble Union Minister for Science and Technology, Environment, Forest and Climate Change and Earth Sciences, Govt. of India visited the Centre for Research and Education in Science and Technology (CREST), Indian Institute of Astrophysics (IIA) at Hosakote. He was welcomed by Prof. P Sreekumar, Director of IIA and Prof. G C Anupama, Dean and Professor-in-charge of CREST and others at CREST.

On 31 May 2017, three space-based observatories – India’s Astrosat, NASA’s Chandra and NASA’s and ESA’s Hubble Space Telescope, along with a ground-based observatory High Accuracy Radial velocity Planet Searcher (HARPS), participated in this exciting exercise and have detected a coronal explosion -- an unusually large release of plasma and magnetic field from a star – in Proxima Centauri.

How do stars and star clusters influence their neighbourhood? How does the birth of stars affect their neighbours? let us start with the birth of a star. It begins with gasses, mostly hydrogen, accumulating under gravity until it gets hot and dense enough to start nuclear fusion, where the lighter Hydrogen atoms merge to form heavier helium atoms, with an enormous outburst of energy. This energy moves in the form of a shockwave, pushing all the excess gas away from the newborn star. For a million years after its birth, high energy radiation from the star continues to push the surrounding gas away. From here the picture gets a little murky as we hadn’t quite understood what happened around a star or a cluster of stars, after the million year mark. Now a new study by researchers from Raman Research Institute (RRI), the Indian Institute of Science (IISc) and P.N Lebedev Physical Institute, Moscow, Russia could throw more light on this issue. They have successfully developed a model to simulate the interaction of a star cluster with its surroundings. The model was then tested for accuracy by comparing it with observations from Tarantula Nebula, a nearby star cluster, where the observations matched closely to the predictions made by the model. Maybe now we can better understand the processes that guide the formation of stars, nebulae and galaxies!