Galactic Debris as a Dark Matter Identifier

Dynamic maps of 12 stellar streams trace paths that are determined by the distribution of mass in the Milky Way. Read more in APS Physics…

This entry was posted in APS Physics and tagged , . Bookmark the permalink.

Leave a Reply

Fill in your details below or click an icon to log in:

WordPress.com Logo

You are commenting using your WordPress.com account. Log Out /  Change )

Twitter picture

You are commenting using your Twitter account. Log Out /  Change )

Facebook photo

You are commenting using your Facebook account. Log Out /  Change )

Connecting to %s