Advertisement

HindustanTimes Sat,25 Oct 2014

Life and Universe

NASA Hubble spots star clusters on collision course
ANI
Washington, August 18, 2012
First Published: 13:09 IST(18/8/2012)
Last Updated: 16:26 IST(18/8/2012)
Remnants from a star that exploded thousands of years ago and created a celestial abstract portrait, as captured in this NASA Hubble space telescope image of the Pencil Nebula. Officially known as NGC 2736, the Pencil Nebula is part of the huge Vela supernova remnant, located in the southern constellation Vela. Reuters/File

Astronomers have caught two clusters full of massive stars that may be in the early stages of merging.

The clusters, which were caught using data from NASA’s Hubble Space Telescope, are 170,000 light-years away in the Large Magellanic Cloud, a small satellite galaxy to our Milky Way.

What at first was thought to be only one cluster in the core of the massive star-forming region 30 Doradus (also known as the Tarantula Nebula) has been found to be a composite of two clusters that differ in age by about one million years.

The entire 30 Doradus complex has been an active star-forming region for 25 million years, and it is currently unknown how much longer this region can continue creating new stars.

Smaller systems that merge into larger ones could help to explain the origin of some of the largest known star clusters.

Lead scientist Elena Sabbi of the Space Telescope Science Institute in Baltimore, Md., and her team began looking at the area while searching for runaway stars, fast-moving stars that have been kicked out of their stellar nurseries where they first formed.

“Stars are supposed to form in clusters, but there are many young stars outside 30 Doradus that could not have formed where they are; they may have been ejected at very high velocity from 30 Doradus itself,” Sabbi said.

She then noticed something unusual about the cluster when looking at the distribution of the low-mass stars detected by Hubble.

It is not spherical, as was expected, but has features somewhat similar to the shape of two merging galaxies where their shapes are elongated by the tidal pull of gravity.

Hubble’s circumstantial evidence for the impending merger comes from seeing an elongated structure in one of the clusters, and from measuring a different age between the two clusters.

According to some models, the giant gas clouds out of which star clusters form may fragment into smaller pieces. Once these small pieces precipitate stars, they might then interact and merge to become a bigger system.

This interaction is what Sabbi and her team think they are observing in 30 Doradus.

Also, there is an unusually large number of high-velocity stars around 30 Doradus. Astronomers believe that these stars, often called “runaway stars” were expelled from the core of 30 Doradus as the result of dynamical interactions.

These interactions are very common during a process called core collapse, in which more-massive stars sink to the center of a cluster by dynamical interactions with lower-mass stars. When many massive stars have reached the core, the core becomes unstable and these massive stars start ejecting each other from the cluster.

The big cluster R136 in the center of the 30 Doradus region is too young to have already experienced a core collapse.

However, since in smaller systems the core collapse is much faster, the large number of runaway stars that has been found in the 30 Doradus region can be better explained if a small cluster has merged into Rs. 136.


Advertisement
Copyright © 2014 HT Media Limited. All Rights Reserved