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Nuclear Transients

Workshop 11

Published online by Cambridge University Press:  29 August 2019

S. Mattila ,
M. J. Graham ,
E. Kankare ,
E. Kool ,
T. Moriya ,
M. Perez-Torres  and
Ł. Wyrzykowski
S. Mattila
Affiliation:
Tuorla observatory, Department of Physics and Astronomy, University of Turku, Finland, email: sepmat@utu.fi
M. J. Graham
Affiliation:
California Institute of Technology, USA
E. Kankare
Affiliation:
Astrophysics Research Centre, Queen’s University Belfast, UK
E. Kool
Affiliation:
Department of Physics and Astronomy, Macquarie University, Australia
T. Moriya
Affiliation:
National Astronomical Observatory of Japan, National Institutes of Natural Sciences, Japan
M. Perez-Torres
Affiliation:
Instituto de Astrofísica de Andaluca (CSIC), Spain
Ł. Wyrzykowski
Affiliation:
Warsaw University Astronomical Observatory, Poland
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Abstract

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Workshop 11 covered the substantial recent progress in studies of supernovæ (SNe), tidal disruption events (TDEs), and other types of luminous transients occurring within the nuclear regions of galaxies. In the past, such transients have largely been missed owing to the substantial extinction of those regions, and to the problems of contrast against the bright (and often complex) nuclear background – or mistaken for normal active galactic nucleus (AGN) variability.

Keywords

Supernovæ: general, accretion disks, black hole physicsgalaxies: active, surveys

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