Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-30T06:25:43.788Z Has data issue: false hasContentIssue false
  • English
  • Français

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: [email protected]
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
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S339: Southern Horizons in Time-Domain Astronomy , November 2017 , pp. 263 - 268
Copyright
© International Astronomical Union 2019 

References

Blanchard, P. K., Nicholl, M., Berger, E., et al. 2017, ApJ, 843, 106CrossRefGoogle Scholar
Dong, S., Shappee, B. J., Prieto, J. L., et al. 2016, Science, 351, 257CrossRefGoogle Scholar
Drake, A.J., Djorgovski, S.G., Mahabal, A., et al. 2011, ApJ, 735, 106CrossRefGoogle Scholar
Filippenko, A. V. 1989, AJ, 97, 726CrossRefGoogle Scholar
Graham, M. J., Djorgovski, S. G., Drake, A. J., et al. 2017, MNRAS, 470, 4112CrossRefGoogle Scholar
Kankare, E., Kotak, R., Mattila, S., et al. 2017, Nature Astronomy, 1, 865CrossRefGoogle Scholar
Kool, E. C., Ryder, S., Kankare, E., Mattila, S. et al. 2018, MNRAS, 473, 5641CrossRefGoogle Scholar
Lawrence, A., Bruce, A. G., MacLeod, C., et al. 2016, MNRAS, 463, 296CrossRefGoogle Scholar
Leloudas, G., Fraser, M., Stone, N. C., et al. 2016, Nature Astronomy, 1, 2CrossRefGoogle Scholar
Mattila, S., et al. 2018, Science, 361, 482Google Scholar
Moriya, T.J., Tanaka, M., Morokuma, T., & Ohsuga, K. 2017, ApJ, 843, L19CrossRefGoogle Scholar
Perez-Torres, M., Romero-Canizales, C., Alberdi, A., & Polatidis, A. 2009, A&A, 507, L17Google Scholar
Wyrzykowski, Ł., Kostrzewa-Rutkowska, Z., Kozołwski, S., et al. 2014, AcA, 64, 197Google Scholar
Wyrzykowski, Ł., Zieliński, M., Kostrzewa-Rutkowska, Z., et al. 2017, MNRAS, 465, L114CrossRefGoogle Scholar