Hubble Zooms in on Two Merging Clusters in Tarantula Nebula

NASA’s Hubble Space Telescope has captured an image of two clusters full of massive stars that may be in the early stages of merging.

This is a Hubble Space Telescope image of a pair of star clusters that are believed to be in the early stages of merging. The clusters lie in the gigantic 30 Doradus Nebula, which is 170,000 light-years from Earth (NASA / ESA / E. Sabbi / ESA / STScI / R. O’Connell / University of Virginia / the Wide Field Camera 3 Science Oversight Committee)

What at first was thought to be only one cluster in the core of the massive star-forming region 30 Doradus, also known the Tarantula Nebula, or NGC 2070, has been found to be a composite of two clusters that differ in age by about one million years. These clusters are 170,000 light-years away in the Large Magellanic Cloud, a small satellite galaxy to our Milky Way.

30 Doradus 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.

An international group of astronomers, using the Wide Field Camera 3 on the Hubble Space Telescope, 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,” said Dr Elena Sabbi, lead scientist at the Space Telescope Science Institute in Baltimore, and lead author of the paper published in the Astrophysical Journal Letters ( version).

Dr Sabbi 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 the astronomers think they are observing in 30 Doradus.

Also, there is an unusually large number of high-velocity stars around 30 Doradus. The team believes 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 R136.

Follow-up studies will look at the area in more detail and on a larger scale to see if any more clusters might be interacting with the ones observed.


Bibliographic information: Sabbi et al. 2012. A double cluster at the core of 30 Doradus. ApJ 754, L37; doi: 10.1088/2041-8205/754/2/L37