Understanding Cygnus X-3 Through Multi-Wavelength StudiesReportar como inadecuado



 Understanding Cygnus X-3 Through Multi-Wavelength Studies


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Cygnus X-3 is a unique microquasar which shows X-ray state changes, strong radio emission, and relativistic jets. It is also an unusual X-ray binary with the mass-donating companion being a high mass star Wolf-Rayet but the orbital modulation as inferred from X-ray emission is only 4.8 hours, a value more common in low-mass systems. It has recently been shown by AGILE and Fermi that Cygnus X-3, is a transient gamma-ray source 100 MeV. To understand the environment, nature, and behavior of Cygnus X-3 multi-wavelength observations are necessary. In this proceedings we present the results achieved so far from multi-wavelength campaigns.



Autor: Michael McCollough; Karri Koljonen; Diana Hannikainen; Guy Pooley; Sergei A. Trushkin; Danny Steeghs; Marco Tavani; Robert Droulans

Fuente: https://archive.org/







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