Discovery and follow-up of the unusual nuclear transient OGLE17aaj

dc.contributor.authorGromadzki M
dc.contributor.authorHamanowicz A
dc.contributor.authorWyrzykowski L
dc.contributor.authorSokolovsky KV
dc.contributor.authorFraser M
dc.contributor.authorKozlowski S
dc.contributor.authorGuillochon J
dc.contributor.authorArcavi I
dc.contributor.authorTrakhtenbrot B
dc.contributor.authorJonker PG
dc.contributor.authorMattila S
dc.contributor.authorUdalski A
dc.contributor.authorSzymanski MK
dc.contributor.authorSoszynski I
dc.contributor.authorPoleski R
dc.contributor.authorPietrukowicz P
dc.contributor.authorSkowron J
dc.contributor.authorMroz P
dc.contributor.authorUlaczyk K
dc.contributor.authorPawlak M
dc.contributor.authorRybicki KA
dc.contributor.authorSollerman J
dc.contributor.authorTaddia F
dc.contributor.authorKostrzewa-Rutkowska Z
dc.contributor.authorOnori F
dc.contributor.authorYoung DR
dc.contributor.authorMaguire K
dc.contributor.authorSmartt SJ
dc.contributor.authorInserra C
dc.contributor.authorGal-Yam A
dc.contributor.authorRau A
dc.contributor.authorChen TW
dc.contributor.authorAngus CR
dc.contributor.authorBuckley DAH
dc.contributor.authorBuckley DAH
dc.contributor.organizationfi=Tuorlan observatorio|en=Tuorla Observatory|
dc.contributor.organization-code1.2.246.10.2458963.20.90670098848
dc.converis.publication-id39595853
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/39595853
dc.date.accessioned2022-10-28T12:47:54Z
dc.date.available2022-10-28T12:47:54Z
dc.description.abstract<p>Aims</p><p>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).</p><p>Methods</p><p>We present the OGLE-IV light curve that covers the slow 60-day-long rise to maximum along with photometric, spectro-scopic, and X-ray follow-up during the first year.</p><p>Results</p><p>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.</p>
dc.identifier.eissn1432-0746
dc.identifier.jour-issn0004-6361
dc.identifier.olddbid179054
dc.identifier.oldhandle10024/162148
dc.identifier.urihttps://www.utupub.fi/handle/11111/32958
dc.identifier.urnURN:NBN:fi-fe2021042825965
dc.language.isoen
dc.okm.affiliatedauthorMattila, Seppo
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeB1 Scientific Journal
dc.publisherEDP SCIENCES S A
dc.publisher.countryFranceen_GB
dc.publisher.countryRanskafi_FI
dc.publisher.country-codeFR
dc.relation.articlenumberARTN L2
dc.relation.doi10.1051/0004-6361/201833682
dc.relation.ispartofjournalAstronomy and Astrophysics
dc.relation.volume622
dc.source.identifierhttps://www.utupub.fi/handle/10024/162148
dc.titleDiscovery and follow-up of the unusual nuclear transient OGLE17aaj
dc.year.issued2019

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