Astronomical Research

Giant Galaxies Die From the Inside Out

29.4.2015 | Astronomers, among them Marcella Carollo, have shown how star formation in "dead" galaxies sputtered out billions of years ago: three billion years after the Big Bang, these galaxies still made stars on their outskirts, but no longer in their interiors. So the decline of star formation started in the cores of the galaxies and then spread outwards.
How did massive elliptical galaxies, common in the modern Universe, quenched their once furious rates of star formation? Colossal galaxies like these, also called spheroids, typically pack in stars ten times as densely in their central regions than in our home galaxy, the Milky Way, and have about ten times its mass.

Astronomers refer to these big galaxies as "red and dead" as they exhibit an ample abundance of ancient red stars, but lack young blue stars and show no evidence of new star formation. The estimated ages of the red stars suggest that their host galaxies ceased to make new stars about ten billion years ago. This shutdown began right at the peak of star formation in the Universe, when many galaxies were still giving birth to stars at a pace about twenty times faster than nowadays.

"Massive dead spheroids contain about half of all the stars that the Universe has produced during its entire life," explains Sandro Tacchella of ETH Zurich in Switzerland, lead author of the current Science paper. "We cannot claim to understand how the Universe evolved and became as we see it today unless we understand how these galaxies come to be."
Graph of galaxy development
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(© ESO)

Graph of galaxy development | Galaxies in the early Universe appear at the left, in the blue regions star formation is in progress. The red regions are "dead", only older and redder stars remain - no more young blue stars are being formed. The resulting giant spheroidal galaxies in the modern Universe appear on the right.

Tacchella and colleagues observed a total of 22 galaxies, spanning a range of masses, from an era about three billion years after the Big Bang. The SINFONI instrument on ESO's Very Large Telescope (VLT) collected light from this sample of galaxies, showing precisely where they were churning out new stars. SINFONI could make these detailed measurements of distant galaxies thanks to its adaptive optics system, which largely cancels out the blurring effects of Earth's atmosphere.

The researchers also trained the Hubble Space Telescope on the same set of galaxies, taking advantage of the telescope's location in space above our planet's distorting atmosphere. Hubble's WFC3 camera snapped images in the near-infrared, revealing the spatial distribution of older stars within the actively star-forming galaxies.

Prof. Marcella Carollo
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Prof. Marcella Carollo
"What is amazing is that SINFONI's adaptive optics system can largely beat down atmospheric effects and gather information on where the new stars are being born, and do so with precisely the same accuracy as Hubble allows for the stellar mass distributions," commented Marcella Carollo, also of ETH Zurich and co-author of the study.
According to the new data, the most massive galaxies in the sample kept up a steady production of new stars in their peripheries. In their bulging, densely packed centres, however, star formation had already stopped.

"The newly demonstrated inside-out nature of star formation shutdown in massive galaxies should shed light on the underlying mechanisms involved, which astronomers have long debated," says Alvio Renzini, Padova Observatory, of the Italian National Institute of Astrophysics.

A leading theory is that star-making materials are scattered by torrents of energy released by a galaxy's central supermassive black hole as it sloppily devours matter. Another idea is that fresh gas stops flowing into a galaxy, starving it of fuel for new stars and transforming it into a red and dead spheroid.

"There are many different theoretical suggestions for the physical mechanisms that led to the death of the massive spheroids," said co-author Natascha Förster Schreiber from the Max Planck Institute for extraterrestrial Physics in Garching, Germany. "Discovering that the quenching of star formation started from the centres and marched its way outwards is a very important step towards understanding how the Universe came to look like it does now."
  (© European Southern Observatory ESO, AcademiaNet)

More information


  • S. Tacchella, C.M. Carollo, A. Renzini, N M. Förster Schreiber, P. Lang, S. Wuyts, G. Cresci, A. Dekel, R. Genzel, S. J. Lilly, C. Mancini, S. Newman, M. Onodera, A. Shapley, L. Tacconi, J. Woo, G. Zamorani: Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang, Science 17 April 2015, Vol. 348 no. 6232 pp. 314-317, DOI: 10.1126/science.1261094


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