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Discovery and follow-up of the unusual nuclear transient OGLE17aaj

  • M. Gromadzki
  • , A. Hamanowicz
  • , L. Wyrzykowski
  • , K. V. Sokolovsky
  • , M. Fraser
  • , Sz Kozłowski
  • , J. Guillochon
  • , I. Arcavi
  • , B. Trakhtenbrot
  • , P. G. Jonker
  • , S. Mattila
  • , A. Udalski
  • , M. K. Szymański
  • , I. Soszyński
  • , R. Poleski
  • , P. Pietrukowicz
  • , J. Skowron
  • , P. Mróz
  • , K. Ulaczyk
  • , M. Pawlak
  • K. A. Rybicki, J. Sollerman, F. Taddia, Z. Kostrzewa-Rutkowska, F. Onori, D. R. Young, K. Maguire, S. J. Smartt, C. Inserra, A. Gal-Yam, A. Rau, T. W. Chen, C. R. Angus, D. A.H. Buckley

Research output: Contribution to journalArticlepeer-review

Abstract

Aims. We report on the discovery and follow-up of a peculiar transient, OGLE17aaj, which occurred in the nucleus of a weakly active galaxy. We investigate whether it can be interpreted as a new candidate for a tidal disruption event (TDE). Methods. We present the OGLE-IV light curve that covers the slow 60-day-long rise to maximum along with photometric, spectroscopic, and X-ray follow-up during the first year. Results. OGLE17aaj is a nuclear transient exhibiting some properties similar to previously found TDEs, including a long rise time, lack of colour-temperature evolution, and high black-body temperature. On the other hand, its narrow emission lines and slow post-peak evolution are different from previously observed TDEs. Its spectrum and light-curve evolution is similar to F01004-2237 and AT 2017bgt. Signatures of historical low-level nuclear variability suggest that OGLE17aaj may instead be related to a new type of accretion event in active super-massive black holes.

Original languageEnglish
Article numberL2
Number of pages5
JournalAstronomy and Astrophysics
Volume622
DOIs
Publication statusPublished - 01 Feb 2019

Keywords

  • Black hole physics
  • Galaxy: nucleus

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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