The high-energy gamma-ray emission discovered using the H.E.S.S. telescopes from the binary system PSR B1259 −63, is modelled using an extension of the approach that successfully predicted it. We find that the simultaneous INTEGRAL and H.E.S.S. data permit both a model with dominant radiative losses, high pulsar wind Lorentz factor and modest efficiency as well as one with dominant adiabatic lo...

Links: [1] https://www.fnb.upc.edu/content/professorat-i-personal-administracio-i-serveis [2] https://www.fnb.upc.edu/node/676 [3] https://www.fnb.upc.edu/normativa [4] https://www.fnb.upc.edu/?q=node/1145 [5] https://www.fnb.upc.edu/node/175 [6] https://www.fnb.upc.edu/?q=node/71 [7] https://www.fnb.upc.edu/node/1259 [8] http://www.ice.upc.edu/ca/innovacio-docent/suport_projectes_institucional...

Links: [1] https://www.fnb.upc.edu/content/professorat-i-personal-dadministraci%C3%B3-i-serveis [2] https://www.fnb.upc.edu/node/676 [3] https://www.fnb.upc.edu/normativa [4] https://www.fnb.upc.edu/?q=node/1145 [5] https://www.fnb.upc.edu/node/175 [6] https://www.fnb.upc.edu/?q=node/71 [7] https://www.fnb.upc.edu/node/1259 [8] http://www.ice.upc.edu/ca/innovacio-docent/suport_projectes_institu...

We report results of CO (J = 1-0) mapping observations of the Wolf-Rayet starburst galaxy Mrk 1259 which has optical evidence for the superwind seen from a nearly pole-on view. The CO emission is detected in the central 4 kpc region. The nuclear CO spectrum shows a blue-shifted (∆V ≃ −27 km s) broad (FWHM ≃ 114 km s) component as well as the narrow one (FWHM ≃ 68 km s). The off-nuclear CO spect...