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by Ajello, M and Albert, A and Atwood, W.B and Barbiellini, G and Bastieri, D and Bechtol, K and Bellazzini, R and Bissaldi, E and Blandford, R.D and Bloom, E.D and Bonino, R and Bottacini, E and Brandt, T.J and Bregeon, J and Bruel, P and Buehler, R and Buson, S and Caliandro, G.A and Cameron, R.A and Caputo, R and Caragiulo, M and Caraveo, P.A and Cecchi, C and Chekhtman, A and Chiang, J and Chiaro, G and Ciprini, S and Cohen-Tanugi, J and Cominsky, L.R and Conrad, J and Cutini, S and D'Ammando, F and De Angelis, A and De Palma, F and Desiante, R and Di Venere, L and Drell, P.S and Favuzzi, C and Ferrara, E.C and Fusco, P and Gargano, F and Gasparrini, D and Giglietto, N and Giommi, P and Giordano, F and Giroletti, M and Glanzman, T and Godfrey, G and Gomez-Vargas, G.A and Grenier, I.A and Guiriec, S and Gustafsson, M and Harding, A.K and Hewitt, J.W and Hill, A.B and Horan, D and Jogler, T and Jóhannesson, G and Johnson, A.S and Kamae, T and Karwin, C and Knödlseder, J and Kuss, M and Larsson, S and Latronico, L and Li, J and Li, L and Longo, F and Loparco, F and Lovellette, M.N and Lubrano, P and Magill, J and Maldera, S and Malyshev, D and Manfreda, A and Mayer, M and Mazziotta, M.N and Michelson, P.F and Mitthumsiri, W and Mizuno, T and Moiseev, A.A and Monzani, M.E and Morselli, A and Moskalenko, I.V and Murgia, S and Nuss, E and Ohno, M and Ohsugi, T and Omodei, N and Orlando, E and Ormes, J.F and Paneque, D and Pesce-Rollins, M and Piron, F and Pivato, G and Porter, T.A and Rainò, S and Rando, R and Razzano, M and Reimer, A and ... and SLAC National Accelerator Lab., Menlo Park, CA (United States) and Partikel- och astropartikelfysik and Skolan för teknikvetenskap (SCI) and KTH and Fysik
Astrophysical Journal, ISSN 0004-637X, 03/2016, Volume 819, Issue 1, p. 44
Journal Article
Journal Article
Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN 1550-7998, 02/2015, Volume 91, Issue 3
With the goal of generating the Galactic Center gamma-ray excess, we revisit models in which the dark matter interacts with the Standard Model through the... 
BREAKING | SEARCH | ASTRONOMY & ASTROPHYSICS | PROTON | EMISSION | BOSONS | PHYSICS, PARTICLES & FIELDS
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2017, Volume 603, p. A89
The central molecular zone (CMZ; inner similar to 200 pc) of the Milky Way is a star formation (SF) environment with very extreme physical properties.... 
Stars: formation | ISM: clouds | Methods: data analysis | H II REGION | methods: data analysis | MAGNETIC-FIELDS | SGR A-ASTERISK | SAGITTARIUS-D | INFRARED-DARK CLOUDS | H2O MASERS | CONTINUUM EMISSION | YOUNG STELLAR OBJECTS | stars: formation | CENTER DUST RIDGE | ASTRONOMY & ASTROPHYSICS | MILKY-WAY | Physics - Astrophysics of Galaxies
Journal Article
Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN 1550-7998, 12/2011, Volume 84, Issue 12
The region surrounding the center of the Milky Way is both astrophysically rich and complex, and is predicted to contain very high densities of dark matter.... 
ABSOLUTE SKY BRIGHTNESS | CONTRACTION | HIGH-ENERGY | ASTRONOMY & ASTROPHYSICS | DIRECTION | LARGE-AREA TELESCOPE | DARK-MATTER | OBSERVABILITY | EMISSION | SUPERMASSIVE BLACK-HOLE | GALAXY | PHYSICS, PARTICLES & FIELDS
Journal Article
Publications of the Astronomical Society of Japan, ISSN 0004-6264, 12/2013, Volume 65, Issue 6, p. 118
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2017, Volume 837, Issue 1, p. 30
Using 25 years of data from uninterrupted monitoring of stellar orbits in the Galactic Center, we present an update of the main results from this unique data... 
techniques: high angular resolution | black hole physics | astrometry | Galaxy: center | Galaxy: fundamental parameters | MILKY | DISTANCE | SGR A-ASTERISK | RESOLUTION | SUPERMASSIVE BLACK-HOLE | GALAXY | ASTRONOMY & ASTROPHYSICS | YOUNG STARS | MASS | EXTINCTION | SINFONI | Physics - Astrophysics of Galaxies
Journal Article
Physical Review Letters, ISSN 0031-9007, 10/2015, Volume 115, Issue 16, p. 161301
We detect a line at 3.539 +/- 0.011 keV in the deep exposure data set of the Galactic center region, observed with the x-ray multi-mirror mission Newton. The... 
KEV STERILE NEUTRINO | X-RAY-LINE | PHYSICS, MULTIDISCIPLINARY | GALAXY CLUSTERS | ROTATION CURVE | SPIRAL GALAXIES | GALACTIC-CENTER | XMM-NEWTON OBSERVATIONS | EMISSION-LINE | SPECTRAL FEATURE | DENSITY PROFILE | Galactic clusters | Origins | Dark matter | X-rays | Consistency | Milky Way Galaxy | Observers | Spectra
Journal Article