Informace o publikaci
Tidal disruption of a low-mass star in an active galactic nucleus as the origin of the PS16dtm outburst
| Autoři | |
|---|---|
| Rok publikování | 2026 |
| Druh | Recenzovaný odborný článek |
| Časopis / Zdroj | ASTRONOMY & ASTROPHYSICS |
| Fakulta / Pracoviště MU | |
| Citace | |
| www | https://www.aanda.org/articles/aa/full_html/2026/08/aa59091-26/aa59091-26.html |
| Doi | https://doi.org/10.1051/0004-6361/202659091 |
| Klíčová slova | accretion; accretion disks; galaxies: active |
| Přiložené soubory | |
| Popis | Context. The event PS16dtm, which occurred in the centre of the narrow-line Seyfert 1 (NLS1) galaxy SDSS J015804.75-005221.8 (z = 0.080440), is one of the few candidates for a tidal disruption event in an already-accreting active galactic nucleus. Aims. We wish to shed light on the character of the tidal disruption event in this source since it exhibits unusual peculiarities, such as the double-peak optical/UV light curve and a low blackbody temperature with a lack of X-ray emission. Methods. We performed a spectral analysis of the source before and during the event. We modelled the time evolution of the luminosity profile using a numerical code that describes the viscous evolution of the flow. Results. Based on the combined spectral and timing studies, we interpret the event as the disruption of a ~0.3 M? main-sequence star or as the gradual partial disruption of a low-mass giant star. The star is likely on a circular orbit, embedded in the accretion disc. We discuss that the evolution of the star rather suggests that the orbit is counter-rotating. We observe the system at a sufficiently large viewing angle that the actual disruption process is not directly observed. The disrupted star and inner disc are shielded from the observer by a gaseous envelope. Further observations of the system as it returns to the previous NLS1 state, particularly in the X-ray band, are needed to confirm the proposed scenario and to place constraints on the return to a regular NLS1 state. |
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