Employing data collected during the first 25 months of observations by the Fermi-LAT, we describe and subsequently seek to model the very high energy (<300 MeV) emission from the central few parsecs of our Galaxy. We analyze the morphological, spectral, a
No takes yet. Share an insight, caveat, or question.
Chernyakova et al. (2010) studied this question.
Synapse has enriched 3 closely related papers on similar clinical questions. Consider them for comparative context: