Rochester Institute of Technology | 2015 July 23
[img3="This image, captured by the Very Large Array, shows the atomic hydrogen distribution of the Whirlpool Galaxy. The “X” marks the dwarf companion satellite. Dynamical simulations can recover its location and mass. (Credit: Chakrabarti et al. 2011)"]http://www.rit.edu/news/pics/WhirlpoolGalaxy.jpg[/img3][hr][/hr]A ripple in the outskirts of the Milky Way—and a hunch—led Rochester Institute of Technology astrophysicist Sukanya Chakrabarti to a previously undetected dwarf galaxy hidden under a veil of dark matter. Now Chakrabarti is refining her technique to uncover dwarf galaxies and understand dark matter by simulating the evolutionary histories of galactic disks, rich in atomic hydrogen, and their satellite populations.
Chakrabarti’s study on these overlapping regions found in spiral galaxies, like the Milky Way, is funded by a three-year $325,053 grant from the National Science Foundation. Her research seeks to solve an astrophysical conundrum dubbed “the missing satellites problem,” in which theoretical simulations that predict an abundance of satellite galaxies are unsupported by observational data.
Earlier this year, Chakrabarti, assistant professor of physics in RIT’s School of Physics and Astronomy, validated her prediction of a previously unseen satellite galaxy located close to the plane of the Milky Way. In her new study, Chakrabarti and Andy Lipnicky, a Ph.D. student in RIT’s astrophysical sciences and technology program, will create the first “mock” map and catalogue of satellite populations from analyzing extended atomic hydrogen disks.
“We will produce models that are consistent with both the atomic hydrogen and stellar data of our galaxy, which displays large ripples in the outskirts, a prominent warp and vertical waves in the galactic disk,” Chakrabarti said. ...
