ICATE 21876
INSTITUTO DE CIENCIAS ASTRONOMICAS, DE LA TIERRA Y DEL ESPACIO
Unidad Ejecutora - UE
artículos
Título:
Modeling the Black Hole Recoil from the Nucleus
Autor/es:
FERRARI, G.; DOTTORI, H.; DIAZ, R. J.
Revista:
Journal of Modern Physics
Editorial:
Scientific Research Publishing
Referencias:
Lugar: Irvine, California; Año: 2013 vol. 4 p. 55 - 63
ISSN:
2153-1196
Resumen:
GEMINI + GMOS and Chandra emission-line spectroscopy reveal that the Fanaroff-Riley II radio-source J133658.3- 295105 is a local object behind the barred-spiral galaxy M83 that is projected onto the galaxy?s disk at about 60" from the galaxy?s optical nucleus. J133658.3-295105 and its radiolobes are aligned with the optical nucleus of M83 and two other radio-sources neither of which are supernova remnants or HII regions. The optical nucleus of M83 is off-centered by 2.7" (~60 pc) with regard to the kinematic center. Its mass is within the range (1 - 4) × 106 Msun and the velocity dispersion at its center points to a non-resolved mass concentration of
