Duo of Titanic Galaxies Captured in Extreme Starbursting Merger

13 November, 2017 / Read time: 6 minutes

New observations with the Atacama Large Millimeter/submillimeter Array (ALMA) have uncovered the never-before-seen close encounter between two astoundingly bright and spectacularly massive galaxies in the early Universe. These so-called hyper-luminous starburst galaxies are exceedingly rare at this epoch of cosmic history — near the time when galaxies first formed — and may represent one of the most-extreme examples of violent star formation ever observed.

Astronomers captured these two interacting galaxies, collectively known as ADFS-27, as they began the gradual process of merging into a single, massive elliptical galaxy. An earlier sideswiping encounter between the two helped to trigger their astounding bursts of star formation. Astronomers speculate that this merger may eventually form the core of an entire galaxy cluster. Galaxy clusters are among the most massive structures in the Universe.

“Finding just one hyper-luminous starburst galaxy is remarkable in itself. Finding two of these rare galaxies in such close proximity is truly astounding,” said Dominik Riechers, an astronomer at Cornell University in Ithaca, New York, and lead author on a paper appearing in the Astrophysical Journal. “Considering their extreme distance from Earth and the frenetic star-forming activity inside each, it’s possible we may be witnessing the most intense galaxy merger known to date.”

The ADFS-27 galaxy pair is located approximately 12.7 billion light-years from Earth in the direction of the Dorado constellation. At this distance, astronomers are viewing this system as it appeared when the Universe was only about one billion years old.

Astronomers first detected this system with the European Space Agency’s Herschel Space Observatory. It appeared as a single red dot in the telescope’s survey of the southern sky. These initial observations suggested that the apparently faint object was in fact both extremely bright and extremely distant. Follow-up observations with the European Southern Observatory's Atacama Pathfinder Experiment (APEX) telescope confirmed these initial interpretations and paved the way for the more detailed ALMA observations.

Artist impression of two starbursting galaxies beginning to merge in the early Universe. Credit: NRAO/AUI/NSF

With its higher resolution and greater sensitivity, ALMA precisely measured the distance to this object and revealed that it was in fact two distinct galaxies. The pairing of otherwise phenomenally rare galaxies suggests that they reside within a particularly dense region of the Universe at that period in its history, the astronomers said.

The new ALMA observations also indicate that the ADFS-27 system has approximately 50 times the amount of star-forming gas as the Milky Way. “Much of this gas will be converted into new stars very quickly,” said Riechers. “Our current observations indicate that these two galaxies are indeed producing stars at a breakneck pace, about one thousand times faster than our home galaxy.”

The galaxies — which would appear as flat, rotating disks — are brimming with extremely bright and massive blue stars. Most of this intense starlight, however, never makes it out of the galaxies themselves; there is simply too much obscuring interstellar dust in each.

This dust absorbs the brilliant starlight, heating up until it glows brightly in infrared light. As this light travels the vast cosmic distances to Earth, the ongoing expansion of the Universe shifts the once infrared light into longer millimeter and submillimeter wavelengths, all thanks to the Doppler effect.

ALMA was specially designed to detect and study light of this nature, which enabled the astronomers to resolve the source of the light into two distinct objects. The observations also show the basic structures of the galaxies, revealing tail-like features that were spun-off during their initial encounter.

Composite image of ADFS-27 galaxy pair. The background image is from ESA's Herschel Space Observatory. The object was then detected by ESO's Atacama Pathfinder Experiment (APEX) telescope (middle image). ALMA (right) was able to identify two galaxies: ADFS-27N (for North) and ADFS-27S (for South). The starbursting galaxies are about 12.8 billion light-years from Earth and destined to merge into a single, massive galaxy. Credit: NRAO/AUI/NSF, B. Saxton; ESA Herschel; ESO APEX; ALMA (ESO/NAOJ/NRAO); D. Riechers

The new observations also indicate that the two galaxies are about 30,000 light-years apart, moving at roughly several hundred kilometers per second relative to each other. As they continue to interact gravitationally, each galaxy will eventually slow and fall toward the other, likely leading to several more close encounters before merging into one massive, elliptical galaxy. The astronomers expect this process to take a few hundred million years.

“Due to their great distance and dustiness, these galaxies remain completely undetected at visible wavelengths,” noted Riechers. “Eventually, we hope to combine the exquisite ALMA data with future infrared observations with NASA’s James Webb Space Telescope. These two telescopes will form an astronomer’s ‘dream team’ to better understand the nature of this and other such exceptionally rare, extreme systems.”

Additional information

This research is presented in a paper titled “Rise of the titans: a dusty, hyper-luminous ‘870 µm riser’ galaxy at z~6,” by D. Riechers, et al., appearing in the Astrophysical Journal.

The team is composed of Dominik A.Riechers (Cornell University, USA); T.K. Daysy Leung (Cornell University, USA); Rob J.Ivison (European Southern Observatory, Germany, and University of Edinburgh, UK) Ismael Pérez-Fournon (Instituto de Astrofisica de Canarias, y Universidad de La Laguna, Spain); Alexander J.R.Lewis (University of Edinburgh, UK); Rui Marques-Chaves (Instituto de Astrofisica de Canarias, y Universidad de La Laguna, Spain); Ivan Oteo (European Southern Observatory, Germany, and University of Edinburgh, UK); Dave L.Clements (Imperial College London, UK); Asantha Cooray (University of California, Irvine, USA); Josh Greenslade (Imperial College London, UK); Paloma Martínez-Navajas (Instituto de Astrofisica de Canarias, y Universidad de La Laguna, Spain); Seb Oliver (University of Sussex, UK); Dimitra Rigopoulou (University of Oxford, UK, and Rutherford Appleton Laboratory, UK); Douglas Scott (University of British Columbia, Canada), and Axel Weiss (Max-Planck-Institut für Radioastronomie, Germany).

The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of the European Organisation for Astronomical Research in the Southern Hemisphere (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 Ministry of Science and Technology (MOST) in Taiwan 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.