The turbulent birth of super star clusters in galaxy mergers

Feb 10, 2012
Photomontage illustrating the discovery of a super star cluster in the Antennae galaxies. Bottom left: landscape image showing the two galaxies interacting, just as they were discovered in the last century Top left: close-up on the central region, where both galaxies interpenetrate. Image obtained by NASA's Hubble telescope. The images on the right-hand side, prepared by Cinthya Herrera, illlustrate the observations carried out by ALMA and VLT. The ALMA image, to the left, shows the clouds containing the youngest and largest star clusters (star symbol). The VLT image, on the right, shows the energy radiation from clouds. The bright compact source in this image (red) is present where two masses of gas moving at very different speeds (in red and blue inside the frame in the bottom right) collide. Observations show that this is where energy loss is at its highest and that conditions are met to form a new cluster within a few million years. Credit: IAS

By combining two of the most advanced telescopes in the world -- the new Atacama Large Millimeter Array (ALMA) and the Very Large Telescope (VLT) of ESO -- a team of French astronomers from the Institut d'astrophysique spatiale (IAS- CNRS) led by graduate student Cinthya Herrera has for the first time traced the very first steps in the formation of young super-star clusters in a nearby galaxy merger, the “Antennae”. This analysis, now published as an Astronomy & Astrophysics letter, not only represents a novel avenue for studying the very early stages of star formation in external galaxies, it is also ALMA's first scientific result ever to be published. It gives a foretaste of how ALMA will revolutionize our views on star formation and galaxy growth.

Mergers of massive, gas-rich galaxies are veritable fireworks of star formation, and many of the stars in galaxies formed during such short, vigorous events, from the early history of the Universe until today.

Such outbursts of star formation, starbursts, trigger the formation of giant clusters of millions of young stars within a few tens of light years. Similar volumes around our own solar system only contain a handful of stars.

Astronomers discovered the first super in the Antennae galaxy merger in images taken with the Hubble Space nearly 20 years ago, but until now, the physical processes which led to their formation were largely unknown. By combining the first data of the Antennae with observations previously obtained at the ESO VLT, the scientists are now able to trace directly how the galaxy merger triggers the formation of super star clusters. This study forms the backbone of Ms. Herrera's thesis work at the IAS in Orsay. A Chilean graduate student, she is doing her PhD thesis in France as part of a bilateral program between the CNRS and CONICYT (Chile). Understanding the astrophysical processes that lead to and galaxy growth is one of the overriding scientific goals of ALMA.

Rather than studying young star clusters after they form, as has been done previously, Ms. Herrera followed a new approach by quantifying the energy lost by the gas in the star-forming clouds of the Antennae. Stars form from gas that is dense and very cold, however, in the Antennae, the galaxy merger stirs up the gas, making it highly turblent. To form new stars, the gas must lose this turbulent energy, so that it can cool, condense, and eventually collapse into a new star cluster.

This immense energy loss, predicted by theory, is now visible by using ALMA and the VLT. As the gas settles into gas clouds, and cools down, it emits a faint glow of light which can be observed with the VLT in the near-infrared. However, seeing this glow alone was not enough. The scientists also had to measure the turbulence in the surrounding gas clouds created by the galaxy merger, which is now  possible with ALMA.

In only one of these clouds, the researchers found a clump of gas, massive enough to form a new super star cluster itself, which is radiating its turbulent energy very rapidly. In this region, where the gravitational pull of the galaxy merger is as its strongest, ALMA only sees an ordinary cloud, which for the is the brightest object in all of the Antennae galaxies. In only a few million years, the blink of an eye in a galaxy's lifetime, this cloud will have lost all its turbulence, and a new cluster will be born. This first example illustrates the plethora of exciting new discoveries that astronomers like Ms. Herrera are hoping to make once ALMA reaches its full capabilities.

Explore further: Image: Galactic wheel of life shines in infrared

More information: ALMA CO and VLT/SINFONI H2 observations of the Antennae overlap region: mass and energy dissipation. Herrera, C. N., et al. 2012, A&A, volume 538, L9.

add to favorites email to friend print save as pdf

Related Stories

Antennae Galaxies

May 19, 2008

This image of the Antennae galaxies is the sharpest yet of this merging pair of galaxies. During the course of the collision, billions of stars will be formed. The brightest and most compact of these star ...

Colliding galaxies make love, not war

Oct 17, 2006

A new Hubble image of the Antennae galaxies is the sharpest yet of this merging pair of galaxies. As the two galaxies smash together, billions of stars are born, mostly in groups and clusters of stars. The ...

Hubble Sees Star Cluster 'Infant Mortality'

Jan 10, 2007

Astronomers have long known that young or "open" star clusters must eventually disrupt and dissolve into the host galaxy. They simply don't have enough gravity to hold them together, unlike their much more ...

Survey Reveals Building Block Process For Biggest Galaxies

Apr 12, 2006

A new study of the universe's most massive galaxy clusters shows how mergers play a critical role in their evolution. Astronomers used the twin Gemini Observatory instruments in Hawaii and Chile, and the Hubble Space Telescope ...

Astronomers Discover Star-Studded Galaxy Tail

Jun 17, 2010

(PhysOrg.com) -- NASA's Galaxy Evolution Explorer has discovered a galaxy tail studded with bright knots of new stars. The tail, which was created as the galaxy IC 3418 plunged into the neighboring Virgo cluster ...

Hubble Eyes Star Birth in the Extreme

Jun 13, 2006

Staring into the crowded, dusty core of two merging galaxies, NASA's Hubble Space Telescope has uncovered a region where star formation has gone wild.

Recommended for you

Image: Galactic wheel of life shines in infrared

6 hours ago

It might look like a spoked wheel or even a "Chakram" weapon wielded by warriors like "Xena," from the fictional TV show, but this ringed galaxy is actually a vast place of stellar life. A newly released ...

New window on the early Universe

Oct 22, 2014

Scientists at the Universities of Bonn and Cardiff see good times approaching for astrophysicists after hatching a new observational strategy to distill detailed information from galaxies at the edge of ...

User comments : 0