Milky-Way-Like Galaxies of the Early Universe –“Were Smaller, Hyper-Star Generating Objects”

 

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Large disk galaxies like our own Milky Way were not always the well-ordered, pinwheel-like, spiral structures we see in the universe today. On the contrary, international experts who specialize in galaxy formation and evolution believe that about 8-to-10 billion years ago, progenitors of the Milky Way and similar disk/spiral galaxies were smaller and less organized, yet highly active in their youth.


In previous NASA and National Science Foundation-funded research, Texas A&M University astronomer Casey Papovich and his collaborators showed that these younger versions of such galaxies were churning out new stars faster than at any other point in their lifespans, suggesting that they must be amazingly rich in star-forming material. And now, they have compelling evidence—the galactic equivalent of a smoking gun.

The image above combines data from ALMA and the Hubble Space Telescope. Shown in red is the distant, background galaxy, being distorted by the gravitational lens effect produced by the galaxy in the foreground, depicted as the blue dot seen by Hubble. The background galaxy appears warped into a so-called Einstein ring: a circle of light around the foreground galaxy. (Dan Marrone)

Using the National Radio Astronomy Observatory’s Atacama Large Millimeter/submillimeter Array (ALMA)—a huge, highly sophisticated radio telescope array situated at 16,500 feet altitude in the high desert of Chile—a Papovich-led team of astronomers studied four very young versions of galaxies like the Milky Way that are 9 billion light-years distant, meaning the team could see them as they looked approximately 9 billion years ago. They discovered that each galaxy was incredibly rich in carbon monoxide—a well-known tracer of molecular gas, which is the fuel for star formation.

“We used ALMA to detect adolescent versions of the Milky Way and found that such galaxies do indeed have much higher amounts of molecular gas, which would fuel rapid star formation,” said Papovich, lead author on the paper and a member of the George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy. “I liken these galaxies to an adolescent human who consumes prodigious amounts of food to fuel their own growth during their teenage years.”

In addition to Papovich, the research team also includes fellow Texas A&M astronomers Ryan Quadri and Kim-Vy Tran, as well as astronomers from Leiden Observatory in Holland, Swinburne University and Macquarie University in Australia, the National Optical Astronomy Observatory (NOAO), the University of Texas at Austin, Lyon Observatory in France and the Max Plank Institute for Astronomy in Germany.

 

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The image of the molecular gas (indicated in red) above, superimposed on Hubble Space Telescope images of the four young Milky Way-like galaxies. These Hubble images are much sharper than the images of the gas from ALMA. Therefore, while the gas appears as a halo here, Papovich says it is more likely to be co-spatial with the starlight in the galaxies. (National Radio Astronomy Observatory)

Though the relative abundance of star-forming gas is extreme in these galaxies, Papovich says they are not yet fully formed and rather small compared to the Milky Way as we see it today. The new ALMA data indicate that the vast majority of the mass in these galaxies is in cold molecular gas rather than in stars—a situation that Papovich says is reversed at present in our Milky Way, where the mass in stars outweighs that in gas by a factor of 10 to 1. These observations, he notes, are helping build a complete picture of how matter in Milky-Way-size galaxies evolved and how our own galaxy formed.

“Most stars today exist in galaxies like the Milky Way, so by studying how galaxies like our own formed, we’ve come to understand the most typical locations of stars in the universe,” said Papovich. “Our current research shows that Milky Way-mass galaxies appear to accumulate most of their gas during their first few billion years of history. At that stage, they have most of the fuel they need to produce the stars they currently encompass in the present.”

The presence of extensive gas reservoirs backs up the team’s previous observations that provided the first tangible pictures showcasing the unprecedented life story of Milky Way galaxy evolution. Among other details, their prior study revealed a stellar birth rate 30 times higher than it is in the Milky Way today—roughly one per year, compared to about 30 each year 9.5 billion years ago.

“Thanks to ALMA and other innovative instruments that allow us to peer 9 billion years into the past to analyze galaxies that are likely similar to the progenitor of our own Milky Way galaxy, we can actually prove what our observations show,” Papovich said. “This will begin to tell us how these galaxies formed stars at such a rapid pace, compared to conditions at present,” he said.

Papovich, Quadri and Tran are among roughly two dozen astronomers around the world who have spent years studying carefully selected distant galaxies similar in mass to the progenitor of our own Milky Way that were found in two deep-sky program surveys of the universe, the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) and the FourStar Galaxy Evolution Survey (ZFOURGE).

Beyond ALMA, the team’s research has used observations from NASA’s Hubble and Spitzer Space Telescopes and the European Space Agency’s Herschel Space Observatory. The Hubble images from the CANDELS survey also provided structural information about galaxy sizes and how they evolved. Far-infrared light observations from Spitzer and Herschel helped the astronomers trace the star-formation rate.

The team’s paper, Large Molecular Gas Reservoirs in Ancestors of Milky Way-Mass Galaxies 9 Billion Years Ago, can be viewed online along with related images and captions.

More information: C. Papovich et al. Large molecular gas reservoirs in ancestors of Milky Way-mass galaxies nine billion years ago, Nature Astronomy (2016). DOI: 10.1038/s41550-016-0003

The Daily Galaxy via Texas A&M University

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