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(gamma et neutrino) au TeV - LUTH

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Galactiques:<br />

Un grande nombre de sources de différents types<br />

● Young Shell type Supernova Remnants<br />

● Older and/or Interacting SNRs<br />

● Composite SNRs<br />

● Pulsar Wind Nebulae (PWN)<br />

● Binary Systems (LS 5039, LSI +61 303)<br />

● Variable PWN in binary<br />

● Open Stellar Clusters<br />

● Galactic Center<br />

● Galactic diffuse emission<br />

● Unidentified sources ...<br />

Extra-galactiques :<br />

● Blazars<br />

● Radiogalaxies (FRI: M87+?)<br />

● Flat Spectrum Radio Quasars (3C 273, recent)<br />

● Extragalactic Background Light (EBL)<br />

● Multiwave-length campains<br />

● Starburst Galaxies (UL)<br />

● GRBs (UL)<br />

● ...<br />

● Un grande nombre de suj<strong>et</strong>s<br />

scientifiques !<br />

13 . 11 . 08 Yvonne Becherini, APC Paris 5

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