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Bulge formation in very late-type galaxies
YanNing Fu, JieHao Huang, ZuGan Deng
The dynamical evolution of super star clusters (SSCs) moving in the background of a dark matter halo has been investigated as a possible event responsible for the formation of bulg…
Polarization of photospheric lines from turbulent dynamo simulations
J. Sánchez Almeida, T. Emonet, F. Cattaneo
We employ the magnetic and velocity fields from turbulent dynamo simulations to synthesize the polarization of a typical photospheric line. The synthetic Stokes profiles have prope…
Timing analysis of the Seyfert-1 galaxy MCG-6-30-15 with XMM-Newton data
N. La Palombara, S. Molendi, J. Wilms +1
We present the main results of a deep timing analysis (in the 0.2-10 keV energy band) of the bright Seyfert-1 galaxy MCG-6-30-15 performed on XMM-Newton data. The light-curves and…
Pulsar Wind Nebulae and Particle Acceleration in the Pulsar Magnetosphere
S. Shibata, M. Tomatsuri, M. Shimanuki +3
This paper deals with the Crab Nebula problem to suggest that particle acceleration takes place not only at the inner shock but also over a larger region in the nebula with disorde…