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LIGHTCURVES OF HST-1 IN M87

The motion of knots in astrophysical jets is commonly interpreted as shock waves moving along it. Observations of the HST-1 knot during extended periods of time have produced complicated light curves on many wavelengths which are difficult to account using standard hydrodynamical models. Here we rep...

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Publié dans:Revista Mexicana de Astronomía y Astrofísica
Auteurs principaux: Y. Coronado, S. Mendoza
Format: Artigo
Langue:Inglês
Publié: Universidad Nacional Autónoma de México 2011
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Accès en ligne:https://www.redalyc.org/articulo.oa?id=57121297018
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