AstroSat reveals how hot stars residing in Milky Way's galaxy clusters evolve

Indian astronomers have peered deep into the Globular Cluster NGC 288, using the Ultraviolet Imaging Telescope (UVIT) on AstroSat to uncover the nature of special kinds of stars. The image of this cluster is the AstroSat ‘Picture of the Month’ for November. AstroSat is India’s first dedicated multi-wavelength space observatory launched by the Indian Space Research Organisation in 2015. Galaxies are made of innumerable stars, some of which are single, like our Sun while others are grouped together in clusters. Our Milky Way has over 150 globular clusters. These are clusters of hundreds of thousands of stars held together by their own gravity, packed into a region just a few tens of light years wide. These globular clusters orbit the centre of the Milky Way as a single unit. NGC 288, located around 30000 light years from the earth is one such Globular Cluster that was imaged by UVIT in three different ‘ultraviolet colours’. “Stars are not unchanging objects. They are born, they evolve through various stages of their life, and then they die,” explains Snehalata Sahu, a PhD student at Bangalore-based Indian Institute of Astrophysics and lead author of the  published paper on the NGC 288 cluster in Monthly Notices of the Royal Astronomical Society. [caption id=“attachment_5648321” align=“alignnone” width=“1280”] NGC 288 has numerous sun-like cooler stars and which make it hard to locate hot stars using optical telescopes. In this image of the same cluster taken though AstroSat’s UV telescope, yellow is the near-UV and white is the far-UV light showing only hot stars as cooler stars become undetectable. Image credit: Snehalata Sahu[/caption] Stars of different masses go through different paths in their evolution. As they do so, their intrinsic luminosity and their surface temperatures (and, therefore, their colours) changes in different ways depending on their mass. Astronomers name different types of stars which are in various phases of their evolution by their location in this luminosity versus temperature plot. The present paper has thrown up interesting results for two such kinds of stars — the Blue Horizontal Branch (BHB) stars and the Blue Straggler (BS) stars in the NGC 288 cluster. All stars in a Globular Cluster are born together and of the same age. They are also about the same distance from us. “Hotter stars are bluer and are bright in the ultraviolet (UV), where they are best studied,” Professor Annapurni Subramaniam, a co-author of the paper, said. UVIT has the unique capability of imaging a large field of view with high resolution. “This helped us not only image the entire cluster up to its outer most regions but also isolate every individual hot star even in the crowded centre of the cluster,” she added. This gave researchers advantage over previous ultraviolet studies of such clusters. They could measure near-UV and far-UV brightness of 115 HB stars, 68 BS stars and 2 Extreme HB (EHB) stars in NGC 288. Combining this data with already known optical properties of these stars, they could accurately model each of these UV-bright stars individually and derive their temperatures as well. [caption id=“attachment_5469561” align=“alignnone” width=“1280”] An artistic rendering of the AstroSat satellite. Image courtesy: ISRO[/caption] “We first looked at the UV properties of the bluer HB stars and could easily distinguish between those stars cooler than 11500 degrees and those that are hotter,” said Sahu. “This change in stellar properties at 11500 degrees is due to atomic diffusion, which alters chemical make-up of outer layers of the star. We have now shown that this break can be easily identified from ultraviolet measurements of these stars and this method can now be used for other clusters as well.” Professor Kameswara Rao, a co-author of the study, explained that the team could calculate the mass and size of the EHB stars as well. “We were able to identify these as sub-dwarf stars, about five times smaller than our Sun, but more than five times hotter. This was possible mainly because we could measure their ultraviolet properties”. The location of stars within a globular cluster change with time as heavier ones settle in the centre. Blue Straggler or BS stars are interesting in themselves. In crowded centres of Globular Clusters, some stars swallow matter from a companion star and sometimes two stars merge to form a new one too. Astronomers believe that BS stars are formed this way, and that’s why their ultraviolet properties are so different. By calculating the mass of each BS star from their ultraviolet data, and by studying their locations in the cluster, researchers could infer the nature of the motion of the stars within the cluster, otherwise known as its dynamical age. “We have now shown that ultraviolet imaging of Globular Clusters is the easiest and clearest way to study the properties of some of these hot stars with peculiar properties. The superior resolution and large field of view of UVIT will prove crucial in understanding the evolution of these kinds of stars,” said Rao.