Elliptical galaxies are large, gas-poor gatherings of older stars and are one of the main types of galaxy along with their spiral and lenticular relatives. Galaxy formation theories suggest that giant elliptical galaxies form from the inside out, with a large core marking the very first stages of formation.
However, evidence of this early construction phase has eluded astronomers — until now.
Astronomers have now spotted a compact galactic core known as GOODS-N-774, and nicknamed Sparky . It is seen as it appeared eleven billion years ago, just three billion years after the Big Bang.
“This core formation process is a phenomenon unique to the early Universe,” explains Erica Nelson of Yale University, USA, lead author of the science paper announcing the results, “we do not see galaxies forming in this way any more. There’s something about the Universe at that time that could form galaxies in this way that it now can’t. We suspect that the Universe could produce denser objects because the Universe as a whole was denser shortly after the Big Bang. It is much less dense now, so it can’t do it anymore.”
Although only a fraction of the size of the Milky Way, the infant galaxy is crammed with so many young stars that it already contains twice as much mass as our entire galaxy. It is thought that the fledgling galaxy will continue to grow, eventually becoming a giant elliptical galaxy. The astronomers think that this barely visible galaxy may be representative of a much larger population of similar objects that are too faint or obscured by dust to be spotted — just like the Sun can appear red and faint behind the smoke of a forest fire.
Alongside determining the galaxy’s size from the Hubble images, the team dug into archival far-infrared images from NASA’s Spitzer Space Telescope and the ESA Herschel Space Observatory to see how fast the compact galaxy is churning out stars. GOODS-N-774 is producing 300 stars per year. “By comparison, the Milky Way produces thirty times fewer than this — roughly ten stars per year,”  says Marijn Franx of Leiden University in the Netherlands, a co-author of the study. “This star-forming rate is really intense!”
This tiny powerhouse contains about twice as many stars as our galaxy, all crammed into a region only 6000 light-years across. The Milky Way is about 100 000 light-years across.
Astronomers believe that this frenzied star formation occurs because the galactic centre is forming deep inside a gravitational well of dark matter, an invisible form of matter that makes up the scaffolding upon which galaxies formed in the early Universe. A torrent of gas is flowing into the well and into the compact galaxy, sparking waves of star birth.
“They’re very extreme environments,” said Nelson. “It’s like a medieval cauldron forging stars. There’s a lot of turbulence, and it’s bubbling. If you were in there, the night sky would be bright with young stars, and there would be a lot of dust, gas, and remnants of exploding stars. To actually see this happening is fascinating.”
The sheer amount of gas and dust within an extreme star-forming region like this may explain why they have eluded astronomers until now. Bursts of star formation create dust, which builds up within the forming core and can block some starlight  — GOODS-N-774 was only just visible, even using the resolution and infrared capabilities of Hubble’s Wide Field Camera 3.
“This galaxy seems to have been furiously forming stars for more than a billion years,” adds Franx. “We have spotted it very early on in its life. Shortly after the time period we’re looking at, we think that this core will have stopped forming stars, and that smaller galaxies will have merged with it over the next 10 billion years until it expanded and grew outwards in size. It would resemble one of the mammoth, sedate ellipticals we see today.”
“We had been searching for this galaxy for years, and it’s very exciting that we finally found it”, says Dokkum, “The big challenge is to understand the physics driving the formation of such objects. The James Webb Space Telescope, Hubble’s successor, will be able to help us find an answer.”
Original release: http://www.eurekalert.org/pub_releases/2014-08/eic-wte082714.php
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