Four
Milky-Way-like progenitor galaxies as seen as they would have appeared 9
billion years ago. ALMA observations of carbon monoxide (red) is
superimposed on images taken with the Hubble Space Telescope. The carbon
monoxide would most likely be suffused throughout the young galaxies. Credit. ALMA (ESO/NAOJ/NRAO) C. Papovich; A. Angelich (NRAO/AUI/NSF); NASA/ESA Hubble Space Telescope
Spiral galaxies like our own Milky Way were not always the well-ordered, pinwheel-like structures we see in the universe today. Astronomers believe that about 8-10 billion years ago, progenitors of the Milky Way and similar spiral galaxies were smaller, less organized, but amazingly rich in star-forming material; so much so, that they would have been veritable star factories, churning out new stars faster than at any other point in their lifetimes. Now, astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have found evidence to support this view. By studying four very young versions of galaxies like the Milky Way as they were seen approximately 9 billion years ago, the astronomers discovered that each galaxy was incredibly rich in carbon monoxide gas, a well-known tracer of star-forming gas. “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 Casey Papovich, an astronomer at Texas A&M University in College Station and lead author on a paper appearing in Nature Astronomy. “I liken these galaxies to an adolescent human who consumes prodigious amounts of food to fuel their own growth during their teenage years.” Though the relative abundance of star-forming gas is extreme in these galaxies, 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. These observations, the astronomers note, are helping build a complete picture of how matter in Milky-Way-size galaxies evolved and how our own galaxy formed.
The National Radio Astronomy Observatory is a facility
of the National Science Foundation, operated under cooperative agreement
by Associated Universities, Inc.
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The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy
facility, is a partnership of ESO, the U.S. National Science Foundation
(NSF) and the National Institutes of Natural Sciences (NINS) of Japan in
cooperation with the Republic of Chile. ALMA is funded by ESO on behalf
of its Member States, by NSF in cooperation with the National Research
Council of Canada (NRC) and the National Science Council of Taiwan (NSC)
and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and
the Korea Astronomy and Space Science Institute (KASI).
ALMA
construction and operations are led by ESO on behalf of its Member
States; by the National Radio Astronomy Observatory (NRAO), managed by
Associated Universities, Inc. (AUI), on behalf of North America; and by
the National Astronomical Observatory of Japan (NAOJ) on behalf of East
Asia. The Joint ALMA Observatory (JAO) provides the unified leadership
and management of the construction, commissioning and operation of ALMA.
The
galaxies in this study and shown in the accompanying image are
identified as ZFOURGE CDFS 467 (top left), ZFOURGE CDFS 4409 (top
right), ZFOURGE CDFS 8193 (bottom left), and ZFOURGE CDFS 6497 (bottom
right).
This research is presented in a paper titled "Large
molecular gas reservoirs in ancestors of Milky Way-mass galaxies nine
billion years ago," by Papovich et al., published in Nature Astronomy. [http://www.nature.com/articles/s41550-016-0003]
Contact:
Charles Blue
NRAO Public Information Officer
+1 434.296.0314; cblue@nrao.edu
