[ad_1]
Pune-based researchers have used the upgraded Giant Metrewave Radio Telescope (uGMRT) — an array of thirty 45-metre antennas unfold over 25 km in Khodad village, Narayangaon, Pune — to supply essentially the most detailed picture but of the galaxy cluster Abell 521.
Galaxy clusters are the most important gravitationally certain methods within the Universe. Detailed photos just like the one now produced helps scientists perceive how galaxy clusters like Abell 521 type and alter over time.
“By studying these faint emissions, scientists can learn about dark matter, magnetic fields and cosmic rays,” stated Ramananda Santra, a PhD candidate at Pune-based National Centre for Radio Astrophysics (NCRA), who alongside together with his information Ruta Kale used the uGMRT telescopes to map the faint constructions from this cluster of galaxies situated about 3 billion gentle years from Earth.
“The upgraded GMRT is super important for finding out more about the faint signals coming from the galaxy cluster in the radio band. These signals are tricky to catch but uGMRT is super sensitive and can pick up these details,” Santra advised The Indian Express.
These galaxy clusters comprise a whole lot to hundreds of galaxies certain collectively by gravity. At the guts of the galaxy clusters lies an unlimited sea of sizzling (with a temperature of tens of hundreds of thousands of kelvin or greater) plasma. The collisions between galaxy clusters launch an enormous quantity of power, which considerably impacts this plasma medium. Abell 521 is one in all such huge giants, well-known for its extremely disturbed medium.
A workforce of astronomers from India, Italy, and the USA used cutting-edge telescopes, which embrace uGMRT, Chandra, and XMM-Newton, and progressive methodologies to make their discovery.
Their findings have been lately printed within the worldwide journal The Astrophysical Journal. The new uGMRT observations led to the invention of latest prolonged radio emission beneath GHz frequencies for the primary time which permits the examine of turbulence and shocks within the plasma. The excessive sensitivity and backbone of GMRT present astronomers with new dimensions to realize data concerning the mysteries of cluster physics, scientists stated.
“Radio Images show beautiful arc-like radio structures at the south of the cluster, and diffuse emission at the cluster center. The X-ray emission, detected by Chandra observatory, reveals a very tight resemblance with the radio structures near the cluster centre. A detailed investigation of the X-ray map reveals a strong connection for the origin of the radio structures via high velocity gas motions during the process of cluster merger,” stated an official readout.
© The Indian Express Pvt Ltd
First uploaded on: 22-02-2024 at 09:29 IST
[adinserter block=”4″]
[ad_2]
Source link