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Multi-messenger astrophysics
Astro-COLIBRI
74 episodes
6 days ago
Discussions around tools and discoveries in the novel domain of multi-messenger and time domain astrophysics. We'll highlight recent publications, discuss tools to faciliate observations and generally talk about the cool science behind the most violent explosions in the universe.
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Astronomy
Science
RSS
All content for Multi-messenger astrophysics is the property of Astro-COLIBRI and is served directly from their servers with no modification, redirects, or rehosting. The podcast is not affiliated with or endorsed by Podjoint in any way.
Discussions around tools and discoveries in the novel domain of multi-messenger and time domain astrophysics. We'll highlight recent publications, discuss tools to faciliate observations and generally talk about the cool science behind the most violent explosions in the universe.
Show more...
Astronomy
Science
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AT2022zod: An Unusual Tidal Disruption Event
Multi-messenger astrophysics
13 minutes 55 seconds
1 month ago
AT2022zod: An Unusual Tidal Disruption Event

**Topic:** Tidal Disruption Events (TDEs) are short-lived optical flares that occur when a black hole shreds a star, offering valuable insight into black hole demographics. This episode dives into the unusual characteristics and implications of the event AT2022zod.


**The Event:**

* AT2022zod was identified as an extreme, short-lived optical flare in an elliptical galaxy at a redshift of 0.11.

* The event lasted roughly 30 days, with a rapid rise time of approximately 13 days.

* It reached a high peak luminosity, positioning it at the extreme end compared to most supernovae.


**The Puzzle:**

* The host galaxy is estimated to contain a massive central Supermassive Black Hole (SMBH) of about $1.0 \times 10^8 M⊙$.

* However, AT2022zod’s short duration and luminosity are **inconsistent** with a TDE powered by this central SMBH.

* Modeling and comparison with other TDEs suggest AT2022zod originated from a lower-mass black hole within the system.

* The event is highly unlikely to be an AGN flare, as it was the only significant flaring activity detected across five years of monitoring. Alternative explanations like kilonovae, compact-binary mergers, and supernovae were also strongly disfavored by the light-curve analysis.


**The Conclusion:**

* Lightcurve modeling points to a Massive Black Hole (MBH) in the **intermediate-mass range** (IMBH, $10^4-10^6 M⊙$) as the source of the disruption.

* The most plausible origin proposed is the tidal disruption of a star by an MBH embedded in an **Ultra-Compact Dwarf galaxy (UCD)** acquired by the host galaxy.

* This discovery highlights the need for flexible search strategies to accommodate unusual events, especially as the Vera C. Rubin Observatory’s Legacy Survey of Space and Time begins.


**Article Reference:**

* Kristen C. Dage et al. (for the COIN collaboration). "AT2022zod: An Unusual Tidal Disruption Event in an Elliptical Galaxy at Redshift 0.11." Draft version December 3, 2025.


Acknowledements: Podcast prepared with Google/NotebookLM. Illustration credits: NASA / CXC / M. Weiss.

Multi-messenger astrophysics
Discussions around tools and discoveries in the novel domain of multi-messenger and time domain astrophysics. We'll highlight recent publications, discuss tools to faciliate observations and generally talk about the cool science behind the most violent explosions in the universe.