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Arc of Blue Stars a Lingering Sign of Shredded Dwarf Galaxy
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Located only 10 million light-years from Earth, Centaurus A is a peculiar-looking galaxy with an extremely dark and wide central dust lane. The combination of this lane and the galaxy’s exterior shell structure implies strongly to astronomers that it is the product of a violent merger between an elliptical galaxy and a smaller companion spiral galaxy. There is compelling evidence that massive Centaurus A ripped apart and swallowed a dwarf irregular galaxy only 200-400 million years ago, leaving behind an arc of young stars stretching at least 2,000 light-years. This finding adds to emerging evidence that smaller galaxies may be significant contributors to the formation of galactic halos, the outer perimeters of galaxies where stellar populations are sparse.  A central black hole is sending out jets in the X-ray and radio spectra.

“The tidal forces of the main galaxy caused a burst of star formation within the infalling galaxy, and what we see now are these young stars spread along the remnant of the incoming orbit,” explains Eric Peng, a graduate student at the Johns Hopkins University in Baltimore. “Though it might appear to be a secondary feature in the complex neighborhood of Centaurus A, this tidal stream is a really sharp illustration of the ongoing process of galactic evolution.”

The arc had been noted as an unusual feature in earlier photographic plates of the violent maelstrom surrounding Centaurus A (also known as Cen A and NGC 5128). However, Peng and his collaborators decided to search for evidence of dwarf-sized fragments near the galaxy by using the powerful ability of modern digital imaging instruments to measure subtle differences in color. This made it possible to isolate the arc, and then to determine its youthful age and dynamic history from independent lines of evidence.

“It was striking how this one arc feature really stood out,” Peng says, “which suggested strongly to us that it had a different origin from its surroundings.”

The spectroscopic data yielded an age for this cluster of approximately 350 million years. Further analysis of the color maps yielded an integrated age for the stream of about 200-400 million years, consistent with a separate estimate for the disruption of the stream based on its physical dynamics.

“We propose that the stream was formed from a tidally triggered burst of star formation that occurred when the dwarf galaxy fell into Cen A about 300 million years ago, which is interesting because it adds to evidence seen in the Milky Way and M31 that galactic halos are built up from the accretion of dwarf satellites,” Peng explains. “However, most of these examples involve older stellar populations in gas-poor dwarf galaxies, whereas the one we’ve observed in Cen A has young stars. This shows that younger, gas-rich dwarfs also fall into galaxies, which has never been seen clearly.”

The stars and star clusters from this tidal stream will eventually disperse into the main body of the galaxy, suggesting that the late infall of gas-rich dwarf galaxies plays an important a role in the build-up of stellar halos, Peng says. This process was likely much more common in the early universe.

“The arc of young stars in Cen A is the closest such feature that we are likely to see the in local universe, so it provides a natural means to study the formation of the stars and star clusters that populate galaxy halos today,” explains CTIO Staff Scientist Knut Olsen.

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