output
19942026
most citedThe 2dF Galaxy Redshift Survey: Spectra and redshifts

2.4k citations

Showing 2012Show all

163 papers · 1 filter

astro-ph.SR2012★ 26 cited

Neutral and ionized gas around the post-Red Supergiant IRC+10420 at au size scales

Rene Oudmaijer, Willem-Jan de Wit

IRC +10420 is one of the few known massive stars in rapid transition from the Red Supergiant phase to the Wolf-Rayet or Luminous Blue Variable phase. The star has an ionised wind a…

astro-ph.HE2012★ 200 cited

Measurement of the extragalactic background light imprint on the spectra of the brightest blazars observed with H.E.S.S

H. E. S. S. Collaboration, :, A. Abramowski +195

The extragalactic background light (EBL) is the diffuse radiation with the second highest energy density in the Universe after the cosmic microwave background. The aim of this stud…

math.LO2012★ 1 cited

On compactifications and the topological dynamics of definable groups

Jakub Gismatullin, Davide Penazzi, Anand Pillay

We discuss definable compactifications and topological dynamics. For G a group definable in some structure M, we define notions of "definable" compactification of G and "definable"…

astro-ph.HE2012★ 102 cited

Constraints on the origin of cosmic rays above eV from large scale anisotropy searches in data of the Pierre Auger Observatory

Pierre Auger Collaboration

A thorough search for large scale anisotropies in the distribution of arrival directions of cosmic rays detected above eV at the Pierre Auger Observatory is reported. For…

astro-ph.SR2012★ 25 cited

The 2.35 year itch of Cyg OB2 #9. II. Radio monitoring

R. Blomme, Y. Naze, D. Volpi +5

Cyg OB2 #9 is one of a small set of non-thermal radio emitting massive O-star binaries. The non-thermal radiation is due to synchrotron emission in the colliding-wind region. Cyg O…

astro-ph.HE2012★ 103 cited

Solution to the Sigma-Problem of Pulsar Wind Nebulae

Oliver Porth, Serguei S. Komissarov, Rony Keppens

We present first results of three dimensional relativistic magnetohydrodynamical simulations of Pulsar Wind Nebulae. They show that the kink instability and magnetic dissipation in…