From Keck: “Prodigious ‘Brightest Cluster Galaxy’ Discovered Churning Trillions of Stars”

Keck Observatory

Keck Observatory

Keck Observatory

Originally September 10, 2015, but not presented.

A massive cluster of galaxies, called SpARCS1049+56, can be seen in this multi-wavelength view from NASA’s Hubble and Spitzer space telescopes. At the middle of the picture is the largest, central member of the family of galaxies (upper right red dot of central pair). Unlike other central galaxies in clusters, this one is bursting with the birth of new stars. Scientists say this star birth was triggered by a collision between a smaller galaxy and the giant, central galaxy. The smaller galaxy’s wispy, shredded parts, called a tidal tail, can be seen coming out below the larger galaxy. Throughout this region are features called “beads on a string,” which are areas where gas has clumped to form new stars. This type of “feeding” mechanism for galaxy clusters — where gas from the merging of galaxies is converted to new stars — is rare. The Hubble data in this image show infrared light with a wavelength of 1 micron in blue, and 1.6 microns in green. The Spitzer data show infrared light of 3.6 microns in red. Credit: NASA/STScI/ESA/JPL-Caltech/McGill

An international team of astronomers has discovered a distant massive galaxy cluster with a core bursting with new stars. The discovery, made with the help of the Maunakea-based W. M. Keck Observatory and Canada-France Hawaii Telescope [CFHT], is the first to show that gigantic galaxies at the centers of massive clusters can grow significantly by feeding off gas stolen from other galaxies. The study has been accepted for publication in The Astrophysical Journal.


“Clusters of galaxies are rare regions of the Universe consisting of hundreds of galaxies containing trillions of stars, as well as hot gas and mysterious dark matter,” said the lead author, Tracy Webb of McGill University, Canada. “The galaxies at the centers of clusters, called Brightest Cluster Galaxies, are the most massive galaxies in the Universe. How they become so huge is not well understood.”

What is so unusual about SpARCS1049+56 is that it is forming stars at a prodigious rate, more than 800 solar masses per year – 800 times faster than in our own Milky Way.

This surprising new discovery was the result of collaborative synergy from ground-based observations from Keck Observatory and CFHT as well as space-based observations from NASA’s Hubble, Spitzer and [ESA]Herschel Space Telescopes.

NASA Hubble Telescope

NASA Spitzer Telescope

ESA Herschel

The Keck Observatory data was gathered by the powerful MOSFIRE infrared spectrograph and was crucial to determining SpARCS1049+56’s distance from Earth as 9.8 billion light-years, that it contains at least 27 galaxies and that it has a total mass equal to about 400 trillion Suns.

MOSFIRE infrared spectrograph

The cluster was first identified from the University of California, Riverside-led, Spitzer Adaptation of the Red-sequence Cluster Survey, or SpARCS, which has discovered about 200 new distant galaxy clusters using deep ground-based optical observations combined with Spitzer Space Telescope infrared observations.

Because Spitzer and Herschel Space Telescopes detect infrared light – enabling observers to see hidden, dusty regions of star formation – they were able to reveal the full extent of the massive amount of star formation going on in SpARCS1049+56. However, the resolution of the infrared observations was insufficient to pinpoint where all this star formation was coming from. Therefore, high-resolution follow-up optical observations were performed by the Hubble Space Telescope to reveal “beads on a string” at the center of SpARCS1049+56 which occur when, similar to a necklace, clumps of new star formation appear strung out like beads on filaments of hydrogen gas.

“Beads on a string” is a telltale sign of something known as a wet merger, which occurs when at least one galaxy in a collision between galaxies is gas rich, and this gas is converted quickly into new stars. The large amount of star formation and the “beads on a string” feature in the core of SpARCS1049+56 are likely the result of the Brightest Cluster Galaxy in the process of gobbling up a gas-rich spiral galaxy.

What is particularly interesting is that Brightest Cluster Galaxies closer to the Milky Way are thought to grow by so-called dry mergers, collisions between gas-poor galaxies that do not result in the formation of new stars. The new discovery is one of the only known cases of a wet merger at the core of a galaxy cluster, and the most distant example ever found.

The team now aims to explore how common this type of growth mechanism is in galaxy clusters. Are there other messy eaters out there similar to SpARCS1049+56, which are also munching on gas-rich galaxies? SpARCS1049+56 may be a rarity or it may be the first of many cases at early times in our Universe when messy eating was the norm.

The Keck Observatory findings were obtained as the result of a collaboration amongst UC faculty members Gillian Wilson (UCR), Michael Cooper(UCI) and Saul Perlmutter (UCB), postdoctoral researcher Brian Hayden (UCB), and graduate students Andrew DeGroot (UCR) and Ryan Foltz (UCR).

“It is very exciting to have discovered such an interesting object,” Wilson said. “Understanding its nature proved to be a real scientific challenge which required the combined efforts of an international team of astronomers and many of the world’s best telescopes to solve.”

The W. M. Keck Observatory operates the largest, most scientifically productive telescopes on Earth. The two, 10-meter optical/infrared telescopes near the summit of Maunakea on the Island of Hawaii feature a suite of advanced instruments including imagers, multi-object spectrographs, high-resolution spectrographs, integral-field spectrographs and world-leading laser guide star adaptive optics systems.

MOSFIRE (Multi-Object Spectrograph for Infrared Exploration) is a highly-efficient instrument that can take images or up to 46 simultaneous spectra. Using a sensitive state-of-the-art detector and electronics system, MOSFIRE obtains observations fainter than any other near infrared spectrograph. MOSFIRE is an excellent tool for studying complex star or galaxy fields, including distant galaxies in the early Universe, as well as star clusters in our own Galaxy. MOSFIRE was made possible by funding provided by the National Science Foundation and astronomy benefactors Gordon and Betty Moore.

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The W. M. Keck Observatory operates the largest, most scientifically productive telescopes on Earth. The two, 10-meter optical/infrared telescopes on the summit of Mauna Kea on the Island of Hawaii feature a suite of advanced instruments including imagers, multi-object spectrographs, high-resolution spectrographs, integral-field spectrometer and world-leading laser guide star adaptive optics systems. Keck Observatory is a private 501(c) 3 non-profit organization and a scientific partnership of the California Institute of Technology, the University of California and NASA.

Today Keck Observatory is supported by both public funding sources and private philanthropy. As a 501(c)3, the organization is managed by the California Association for Research in Astronomy (CARA), whose Board of Directors includes representatives from the California Institute of Technology and the University of California, with liaisons to the board from NASA and the Keck Foundation.
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