From UC Riverside: “UCR astronomers get best measure yet of how fast star formation stopped in galaxy clusters in the early universe”

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From UC Riverside

UC Riverside-led study provides new insight into why galaxies stop forming stars.

This image, taken by NASA’s Hubble Space Telescope, shows galaxy cluster SDSS J0333+0651. (Credit: NASA/ESA Hubble)

Clusters of galaxies are rare regions of the universe consisting of hundreds of galaxies containing trillions of stars, as well as hot gas and dark matter. It has long been known that when a galaxy falls into a cluster, star formation is fairly rapidly shut off in a process known as “quenching.” What actually causes the stars to quench, however, is a mystery, despite several plausible explanations having been proposed by astronomers.

A new international study led by astronomer Ryan Foltz, a former graduate student at the University of California, Riverside, has made the best measurement yet of the quenching timescale, measuring how it varies across 70 percent of the history of the universe. The study has also revealed the process which is likely responsible for shutting down star formation in clusters.

Each galaxy infalling into a cluster is known to bring some cold gas with it which has not yet formed stars.

The Tadpole Galaxy is a disrupted spiral galaxy showing streams of gas stripped by gravitational interaction with another galaxy. Molecular gas is the required ingredient to form stars in galaxies in the early universe. Credit: Hubble Legacy Archive, ESA, NASA and Bill Snyder.

One possibility that has been suggested is that, before it could turn into stars, this cold gas fuel was “stripped” away from the galaxy by the hot, dense gas already in the cluster, causing star formation to cease.

Another possibility is that galaxies were instead “strangled,” that is, they stopped forming stars because their reservoirs ceased getting replenished with additional cold gas once they fell inside the cluster. This is predicted to be a slower process than stripping.

A third possibility is that energy from the star formation itself drove much of the cold gas fuel away from the galaxy and prevented it from forming new stars. This “outflow” scenario is predicted to occur on a faster timescale than stripping, because the gas is lost forever to the galaxy and is unavailable to form new stars.

Because these three different physical processes predict galaxies to quench on different relative timescales over the history of the universe, astronomers have long known that if they could compare the number of quenched galaxies observed over a long time-baseline, the dominant process causing stars to quench would more readily become apparent. The problem: until recently, it was very difficult to find distant clusters, never mind measure the properties of their galaxies. The international Spitzer Adaptation of the Red-sequence Cluster Survey, or SpARCS, survey has now made a measurement of more than 70 percent of the history of the universe, accomplished by pioneering new cluster detection techniques which enabled the discovery of hundreds of new clusters in the distant universe.

Color images of the central regions of z > 1.35 SpARCS clusters. Cluster members are marked with white squares. Credit: SpARCS collaboration.

Using some of their own newly-discovered SpARCS clusters, the new UCR-led study discovered that it takes a galaxy longer to stop forming stars as the universe gets older: only 1.1 billion years when the universe is young (4 billion years old), 1.3 billion years when the universe is middle-aged (6 billion years old), and 5 billion years in the present-day universe.

“Comparing observations of the quenching timescale in galaxies in clusters in the distant universe to those in the nearby universe, revealed that a dynamical process such as gas stripping is a better fit to the predictions than strangulation or outflows,” said Foltz.

To make this state-of-the art measurement, the SpARCS team required 10 nights of observations with the W. M. Keck Observatory telescopes (10 meters in diameter) in Hawaii, and 25 nights of observations with the twin Gemini telescopes (8 meters in diameter) in Hawaii and Chile.

Keck Observatory, Maunakea, Hawaii, USA.4,207 m (13,802 ft), above sea level, showing also NASA’s IRTF and NAOJ Subaru

Gemini South telescope, Cerro Tololo Inter-American Observatory (CTIO) campus near La Serena, Chile, at an altitude of 7200 feet

Gemini/North telescope at Maunakea, Hawaii, USA,4,207 m (13,802 ft) above sea level

“Thanks to the phenomenal investment in our work by these observatories, we now believe we have a good idea of how star formation stops in the most massive galaxies in clusters,” said Gillian Wilson, professor of physics and astronomy at UCR and leader of the SpARCS survey, in whose lab Foltz worked when the study was done. “There are good reasons, however, to believe that lower-mass galaxies may quench by a different process. That is one of the questions our team is working on answering next.”

The team has been awarded 50 additional nights of Gemini time and a $1.2 million grant from the National Science Foundation to study how star formation stops in more regular-mass galaxies. Wilson was also awarded Hubble Space Telescope observations and a NASA grant to analyze high-resolution images of the quenching galaxies.

NASA/ESA Hubble Telescope

The research paper will be published in The Astrophysical Journal.

The W. M. 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). Other authors involved in the study were Adam Muzzin (University of York, Canada), Julie Nantais (Andres Bello University, Chile), Remco van der Burg (European Southern Observatory, Germany), Pierluigi Cerulo (Universidad de Concepción, Chile), Jeffrey Chan (UCR), Sean Fillingham (UCI), Jason Surace (California Institute of Technology), Tracy Webb (McGill University, Canada), Allison Noble (MIT), Mark Lacy (National Radio Astronomy Observatory), Michael McDonald (MIT), Gregory Rudnick (University of Kansas), Ricardo Demarco (Universidad de Concepción, Chile), Christopher Lidman (Australian Astronomical Observatory), Julie Hlavacek-Larrondo (University of Montreal), Howard Yee (University of Toronto, Canada), and Brian Hayden (UCB).

The study was supported by grants from NSF and NASA.

See the full article here .


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