Cargando…
Gamma-ray flares from relativistic magnetic reconnection in the jet of the quasar 3C 279
Spinning black holes in the centres of galaxies can release powerful magnetised jets. When the jets are observed at angles of less than a few degrees to the line-of-sight, they are called blazars, showing variable non-thermal emission across the electromagnetic spectrum from radio waves to gamma ray...
Autores principales: | Shukla, A., Mannheim, K. |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2020
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7442797/ https://www.ncbi.nlm.nih.gov/pubmed/32826906 http://dx.doi.org/10.1038/s41467-020-17912-z |
Ejemplares similares
-
COMPTEL observations of the quasars 3C 273 and 3C 279
por: Williams, O R, et al.
Publicado: (1994) -
COMPTEL gamma-ray observations of the quasars CTA 102 and 3C 454.3
por: Blom, J J, et al.
Publicado: (1994) -
Relativistic beaming and orientation effects in core-dominated quasars
por: Ubachukwu, A A, et al.
Publicado: (2002) -
The Jet Paradigm: From Microquasars to Quasars
por: Belloni, Tomaso
Publicado: (2010) -
Gamma-ray halo around 3C 279: looking through the Sun on the 8th of October
por: Fairbairn, M, et al.
Publicado: (2008)