India's Dedicated Space Telescope AstroSat Spots Rare Hot Ultraviolet-Bright Stars In Milky Way Galaxy
India's Dedicated Space Telescope AstroSat Spots Rare Hot Ultraviolet-Bright Stars In Milky Way GalaxyA false colour image of the globular cluster NGC 2808 obtained using AstroSat/UVIT. The stars as seen using far-UV (FUV) filter are shown in blue colour, and the yellow colour is used to show the stars observed in near-UV (NUV) (Pic Via PIB)

The ultraviolet imaging telescope of the Astrosat, India's first dedicated multi-wavelength space satellite, has spotted rare hot ultraviolet-bright stars in the Milky Way galaxy, a Ministry of Science and Technology statement said on Thursday (21 January).

These stars whose inner core is almost exposed, making them very hot, exist in the late stages of evolution of a Sun-like star. It is not clear how these stars end their lives as not many of them are detected in these fast-evolving phases, making their study crucial, the ministry said.

With spectacular ultraviolet images of the cluster from Ultraviolet Imaging Telescope (UVIT) onboard India’s first multi-wavelength space satellite, AstroSat, the scientists at the Indian Institute of Astrophysics (IIA) distinguished the hot UV-bright stars from the relatively cooler red giant and main-sequence stars which appear dim in these images.

The findings of this study have been accepted for publication in the journal ‘The Astrophysical Journal’.

Motivated by the fact that old globular clusters referred to as dinosaurs of the universe present excellent laboratories where astronomers can understand how stars evolve through various phases between their birth and death, the scientists at IIA looked out for NGC 2808, a massive globular cluster in the Milky Way galaxy.

The team of scientists comprising Deepthi S Prabhu, Annapurni Subramaniam and Snehalata Sahu from IIA combined the UVIT data with observations made using other space missions such as the Hubble Space Telescope and the Gaia telescope along with ground-based optical observations.

About 34 UV-bright stars were found to be members of the globular cluster. From the data, the team derived the properties of these stars such as their surface temperatures, luminosities and radii, the ministry said.

One of the UV-bright stars was found to be about 3000 times brighter than the Sun with a surface temperature of about 100,000 Kelvin.

The properties of these stars were then used to place them on what astronomers call the Hertzsprung-Russel (HR) diagram along with theoretical models to throw light on the characteristics of their parent stars and to predict their future evolution.

Most of the stars were found to have evolved from a solar stage called the horizontal branch stars with hardly any outer envelope. Thus, they were bound to skip the last major phase of life called the asymptotic giant phase and directly become dead remnants or white dwarfs.

Such UV-bright stars are speculated to be the reason for the ultraviolet radiation coming from old stellar systems such as elliptical galaxies which are devoid of young blue stars. Hence, it is all the more important to observe more such stars to understand their properties, the ministry added.

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