archives

gamma rays

This tag is associated with 6 posts
http://fermi.gsfc.nasa.gov/

Gamma-rays from the Galactic Center, a dark matter

For a few years now, excess emission of gamma-rays in the direction of the Galactic Center has puzzled scientists. In the paper we discuss today, the authors re-analyze data from the Fermi telescope to get new insights into the origin of this excess emission. They make the case for the signal being described by dark matter particles annihilating in the center of our Galaxy.

An Unexpected Guest: Fermi-LAT Sees More Novae in Gamma Rays

In 2010 the Fermi-LAT reported a surprising discovery: detection of a gamma ray transient that appeared to come from a nova, V407 Cyg. Since V407 Cyg is a special type of nova, however, it was considered a one-off event. Now two other classical novae have also been found in gamma rays.

Is the Moon polluting your gamma-ray data?

I’m going to go ahead and give away the punchline: the answer to this post’s title is, “If your source is within 8 degrees of the Moon, quite probably.” — at least according to this paper’s authors. Read on to find out why!

An Off-Kilter Galaxy: Separating the DM Peak and the Dynamical Center of the Milky Way

As Astrobites reported a couple of months ago, the Fermi-LAT gamma-ray telescope has reported an anomalous peak at 130 GeV, which could be the long-sought annihilation signature of dark matter. However, one of the strongest critiques of this potential discovery is that the signal is not coming from Sgr A*, the dynamical center of the Milky Way, but rather from about 200 parsecs away. Kuhlen et al. challenge the idea that the dark matter peak must be located at the dynamical center, and find that the combined dark matter-baryonic matter simulation Eris shows a well-defined, consistent offset between its dark matter peak and dynamical center.

X Marks the Spot, said the Gamma Ray

A Fermi/LAT study of the ISM using gamma rays finds evidence for missing gas and variations in the CO-to-molecular gas conversion factor.

The first detected signature of dark matter annihilation?

A flurry of recent papers point to detection of a ~130 GeV gamma-ray emission line from near the Galactic center. If real, this could be the first detection of a signature of annihilating dark matter.

Want an Astrobites t-shirt?

Enter the Astrobites reader survey to help us focus our content and style to serve you best. You could win a free Astrobites t-shirt!

Follow us on Twitter

Like us on Facebook

Astroplots

    http://astrobites.tumblr.com/post/65549158012http://astrobites.tumblr.com/post/62345439779http://astrobites.tumblr.com/post/60939853775http://astrobites.tumblr.com/post/59050954779Visit Astroplots to explore astronomy research through data representation.

Archives

Enter your email address to subscribe to Astrobites and receive notifications of new posts by email.