AT 2021ont (ZTF21abdmevk) was discovered by the Zwicky Transient Facility in the nucleus of a z=0.028 galaxy on June 3, and it is currently rising. An archival SDSS spectrum of the host galaxy, SDSS J162642.49+390842.8, taken in April 2003 indicates a starburst galaxy, with prominent, narrow Balmer and forbidden emission lines.
We obtained an optical spectrum with the SPRAT instrument mounted on the Liverpool Telescope (through OPTICON program OL21A01, PI: Arcavi) at 2021-06-06 23:25:23 UT. The SPRAT spectrum shows a bluer continuum compared to the SDSS spectrum, a significantly higher Hbeta / [OIII]5007 line ratio, and a new emission feature around rest-frame 4680A, consistent with a blend of HeII 4686A and NIII 4640A emission lines. These characteristics have been previously associated with Bowen Fluorescence Flares (BFFs) - a class of enhanced accretion events around supermassive black holes (Trakhtenbrot et al. 2019, Nature Astronomy, 3, 242), likely driven by intense EUV flares that lead to the excitation of the Bowen Fluorescence cascades.
We are pursuing additional spectroscopic and multi-wavelength observations of AT 2021ont.
Catalog | Name | Reported RA | Reported DEC | Reported Obj-Type | Reported Redshift | Host Name | Host Redshift | Remarks | TNS RA | TNS DEC | TNS Obj-Type | TNS Redshift |
---|---|---|---|---|---|---|---|---|---|---|---|---|
TNS | 2021ont [ZTF21abdmevk] | 16:26:42.485 | +39:08:42.86 | 0.028 | WISE J162642.49+390842.7 | 0.02834 | 16:26:42.534 | +39:08:42.96 | SN II | 0.02833 |
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