A dazzling new photo from the NASA/ESA Hubble Space Telescope shows the luminous blue compact galaxy ESO 185-IG013, which is found in the constellation Telescopium.
Thank you for reading this post, don't forget to subscribe!ESO 185-IG013 is located approximately 260 million light-years away in the small southern constellation of Telescopium.
Also known as LEDA 63618, the galaxy is classified as a luminous blue compact galaxy (BCG).
All of the stars in ESO 185-IG013 have a combined mass more than 7 billion solar masses.
“BCGs are nearby galaxies that show an intense burst of star formation,” the Hubble astronomers said in a statement.
“They are unusually blue in visible light, which sets them apart from other high-starburst galaxies that emit more infrared light.”
“We study BCGs because they provide a relatively close-by equivalent for galaxies from the early Universe.”
“This means that BCGs can help us learn about galaxy formation and evolution that may have been happening billions of years ago.”
The astronomers imaged ESO 185-IG013 in ultraviolet, visible, and infrared wavelengths to reveal details about its past.
“Hundreds of young star clusters, many of which are younger than 100 million years, populate the galaxy,” the astronomers said.
“A large number of star clusters are only 3.5 million years old — relative infants compared to the timescale of our Universe.”
“Scientists predict that many of these youngest clusters will not last, since young clusters can often perish after expelling too much of their gas.”
“The large number of young star clusters indicates that ESO 185-IG013 was part of a recent galaxy collision and merger.”
“The perturbed structure of the galaxy, which likely occurred from the violent interactions of gas and dust during the collision, is another sign.”
“The merger supplied the system with lots of fuel for star formation, which continues to take place today.”
“ESO 185-IG013 also contains a tidal shell, the diffuse glow surrounding its bright center, which is a common signal of galaxy mergers,” they said.
“We believe that in a galaxy merger, the smaller of the two interacting galaxies gets disrupted by the larger galaxy, losing most of its material.”
“This releases the material, which then gets pulled in again by the gravity of the larger galaxy.”
“The dense area where the material gets repositioned is called the shell, and it contains many star clusters. In addition to the shell, ESO 185-IG013 boasts a tail of gas in the northeast.”