ar X iv : a st ro - p h / 00 02 43 9 v 1 2 3 Fe b 20 00 C 32 , A Young Star Cluster in IC 1613

ar X iv : a st ro - p h / 00 02 43 1 v 1 2 3 Fe b 20 00 CONSTRAINTS TO THE SSC MODEL FOR MKN 501

We fit the SEDs of the TeV blazar Mkn 501 adopting the homogeneous SynchrotronSelf Compton model to simultaneous X-ray and TeV spectra recently become available. We present detailed model spectra calculated with the above constraints and taking into account the absorption of TeV photons by the IR background. We found that the curved TeV spectra can be naturally reproduced even without IRB absor...

RTES-03 Interfaces.indd

[ B ur ns 20 07 ] B u rn s, A & W el lin gs , A C o n cu rr en t a n d R ea l-T im e Pr o gr am m in g in A d a, e d it io n C am b ri d ge U n iv er si ty P re ss 2 00 7 [ M o to ro la 19 96 ] M o to ro la Ti m e Pr o ce ss in g U n it R ef er en ce M an u al 1 99 6 p p . 1 -1 42 [ M o to ro la 20 00 ] M o to ro la M PC 56 5 & M PC 56 6 2 00 0 p p . 1 -1 31 2 [ P ea co ck 19 97 ] Pe ac o ck , ...

ar X iv : a st ro - p h / 06 10 86 3 v 1 2 9 O ct 2 00 6 The Not So Extraordinary Globular Cluster M 31 037 – B 327 1

A velocity dispersion has been measured for the luminous globular cluster M31 037–B327, claimed to be the most massive star cluster in the Local Group and to be a young “super star cluster” that has survived to an old age. M31 037– B327 has a mass comparable to that of M31 G1, but not significantly larger. Although near the upper end for the mass distribution of globular clusters, it is not an ...

ar X iv : a st ro - p h / 02 12 57 9 v 1 3 1 D ec 2 00 2 Behaviour of Magnetic Tubes in Neutron Star ’ s

It is found from Maxwell's equations that the magnetic field lines are good analogues of relativistic strings. It is shown that the super-conducting current in the neutron star's interior causes local rotation of magnetic flux tubes carrying quantized flux.

ar X iv : a st ro - p h / 02 10 42 8 v 1 1 8 O ct 2 00 2 Star Clusters in Interacting Galaxies : The Case of M 51 Nate