Among galaxies, a voracious flea
Even a dwarf galaxy with very low mass is capable of accreting smaller nearby galaxies, according to an international team of astronomers led by Francesca Annibali of INAF, the Italian National Institute for Astrophysics. This result has been achieved thanks to observations of the region surrounding the dwarf galaxy DDO 68, which has a total stellar mass of only 100 million solar masses, roughly one thousandth of the Milky Way.
In the new study, Annibali and collaborators took advantage of the sensitivity and the large field of view of the Large Binocular Telescope, or LBT, located on Mt. Graham in southeastern Arizona (U.S.). The team discovered that DDO 68, a dwarf galaxy located in an isolated region of space defined as a "void," is actually surrounded by a number of smaller satellite galaxies, and is accreting them.
"In a way, what we saw reminded us of a quote by Jonathan Swift," Annibali said. "'So, naturalists observe, a flea has smaller fleas that on him prey; and these have smaller still to bite 'em; and so proceed ad infinitum.' It turns out that even the smallest of galaxies feed on companions that are even smaller, and so our paper bears that quote in its title."
DDO 68 is one of three known least-evolved galaxies among those that still form stars, with a chemical composition similar to predictions of the Big Bang. Scientists had already thought that its extremely irregular morphology—with a long tail hosting both stars and gas—could be due to tidal effects resulting from gravitational interactions with other bodies. Incidentally, a candidate companion— possibly another small galaxy or a gas cloud—was spotted at a relatively large distance two years ago by a team led by John Cannon of Macalaster College in Minnesota.
|A close-up view of DDO 68 [Credit: Francesca Annibali/INAF]|
LBT's wide, deep images revealed that DDO 68 has a small, incoming stream in addition to its well-known long tail, and is orbited by a few other star and gas companions that are most likely satellites whose ultimate fate is to be accreted. The stream and satellites probably have about 100,000 solar masses – similar to, or even lower than, those of the ultra-faint Milky Way satellites, the least luminous and smallest galaxies known, believed to be the closest local analogs of the first galaxies in the universe.
"Our colleagues, Luca Ciotti and Carlo Nipoti of the Physics and Astronomy Department at the Bologna University, have computed numerical dynamical models of DDO 68's system that reproduce very well the observed configuration of the 'flea with its smaller fleas,'" Annibali said. "This is the first evidence of a stellar stream around an isolated dwarf galaxy of only a hundred million solar masses, and the observational proof that hierarchical galaxy formation processes also work at the smallest scales."
"In other words, not only massive bodies cannibalize smaller ones that happen to lie in their surroundings, but the same appetite and digestion capabilities can be found in the smaller ones," said Monica Tosi, INAF astronomer and member of Annibali's team.
|This image taken in visible light (g band) reveals features of the dwarf galaxy telling of its encounter |
with other, nearby objects [Credit: Francesca Annibali/INAF]
"It is very interesting to discover that a system whose gravitational potential is too low to retain ejecta from supernovae is still capable of attracting and accreting smaller galaxies," Tosi said. "Specific dynamical and hydrodynamical studies are necessary to understand what main mechanisms are at play here."
"The results achieved with DDO 68 show the high discovery power of wide-field instrumentation mounted on 8- to 10-meter class telescopes for future projects devoted to the search of substructures around isolated dwarf galaxies," she said. "It also emphasizes the importance of combining deep observations with theoretical studies on the evolution and the dynamics of both stars and gas in the galaxies we study."
Source: Large Binocular Telescope [August 10, 2016]