Structure, behavior better explained by galaxy collisions
Dwarf galaxies that orbit the Milky Way and the Andromeda galaxies defy the accepted model of galaxy formation, and recent attempts to wedge them into the model are flawed, reports an international team of astrophysicists.
An optical image of the "Tadpole" galaxy, an interacting galaxy, taken by the Hubble Space Telescope. Material stripped from the galaxy during its collision with a smaller galaxy (seen in the upper left corner of the larger interaction partner) forms a long tidal tail. Young blue stars, star clusters and tidal dwarf galaxies are born in these tidal debris. These objects move in a common direction within a plane defined by the orientation and motion of their tidal tail. A similar galaxy interaction might have occurred in the Local Group in the past, which could explain the distribution of dwarf galaxies in co-rotating planes.
Credit: NASA, Holland Ford (JHU), the ACS Science Team and ESA
David Merritt, professor of astrophysics at Rochester Institute of Technology, co-authored "Co-orbiting satellite galaxy structures are still in conflict with the distribution of primordial dwarf galaxies," to be published in an upcoming issue of Monthly Notices of the Royal Astronomical Society. A pre-print of the paper is available online at http://arxiv.org/abs/1406.1799.
The study pokes holes in the current understanding of galaxy formation and questions the accepted model of the origin and evolution of the universe. According to the standard paradigm, 23 percent of the mass of the universe is shaped by invisible particles known as dark matter.
"The model predicts that dwarf galaxies should form inside of small clumps of dark matter and that these clumps should be distributed randomly about their parent galaxy," Merritt said. "But what is observed is very different. The dwarf galaxies belonging to the Milky Way and Andromeda are seen to be orbiting in huge, thin disk-like structures."
The study, led by Marcel Pawlowski at Case Western Reserve University, critiques three recent papers by different international teams, all of which concluded that the satellite galaxies support the standard model. The critique by Merritt and his colleagues found "serious issues" with all three studies.
The team of 14 scientists from six different countries replicated the earlier analyses using the same data and cosmological simulations and came up with much lower probabilities—roughly one tenth of a percent—that such structures would be seen in the Milky Way and the Andromeda galaxy.
"The earlier papers found structures in the simulations that no one would say really looked very much like the observed planar structures," said Merritt.
In their paper, Merritt and his co-authors write that, "Either the selection of model satellites is different from that of the observed ones, or an incomplete set of observational constraints has been considered, or the observed satellite distribution is inconsistent with basic assumptions. Once these issues have been addressed, the conclusions are different: Features like the observed planar structures are very rare."
The standard cosmological model is the frame of reference for many generations of scientists, some of whom are beginning to question its ability to accurately reproduce what is observed in the nearby universe. Merritt counts himself among the small and growing group that is questioning the accepted paradigm.
"Our conclusion tends to favor an alternate, and much older, model: that the satellites were pulled out from another galaxy when it interacted with the Local Group galaxies in the distant past," he said. "This 'tidal' model can naturally explain why the observed satellites are orbiting in thin disks."
Scientific progress embraces challenges to upheld theories and models for a reason, Merritt notes.
"When you have a clear contradiction like this, you ought to focus on it," Merritt said. "This is how progress in science is made."
CONTACT: David Merritt can be reached at email@example.com or 585-730-3847.
IMAGE: An optical image of the "Tadpole" galaxy, an interacting galaxy, taken by the Hubble Space Telescope. Material stripped from the galaxy during its collision with a smaller galaxy (seen in the upper left corner of the larger interaction partner) forms a long tidal tail. Young blue stars, star clusters and tidal dwarf galaxies are born in these tidal debris. These objects move in a common direction within a plane defined by the orientation and motion of their tidal tail. A similar galaxy interaction might have occurred in the Local Group in the past, which could explain the distribution of dwarf galaxies in co-rotating planes.
UGC 10214 ("The Tadpole"): http://www.spacetelescope.org/images/heic0206a/
Credit: NASA, Holland Ford (JHU), the ACS Science Team and ESA
MOVIE: Movie of a computer simulation modeling the merger of two galaxies. The remnant galaxy is similar to our neighboring Andromeda galaxy. Debris from the collision is expelled in long tidal tails, along which tidal dwarf galaxies form. These orbit in a common plane, because they follow the motion of the tidal tail. This might explain the satellite galaxy planes around the Milky Way and Andromeda.
Credit: Observatoire de Paris / GEPI / François Hammer et al.
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