Galactic Archaeology of the Sagittarius Stream
Observations of stars today can reveal billions of years of history.
Observations of stars today can reveal billions of years of history.
The discovery of carbon-rich Mira variables in the Galactic centre could imply the existence of a number of young stars among the otherwise old Galactic bulge population.
Can we hunt down invisible dark matter halos around the Milky Way using the evidence they leave behind as they pass through stellar streams?
Abundance analysis, or chemical tagging, is widely use to identify stars with a common birth. But is a similar abundance alone enough to identify siblings? Can’t stars have doppelgangers?
Do the Milky Way’s satellite galaxies have their own satellites?
The halo of the Milky Way is old. You’ve probably heard that a million times. But can we know more about its age than simply “it’s old”? Yes, we can — and that leads to interesting results!
Image credits: NASA/CXC/M.Weiss/Ohio State/A Gupta et al.