Cargo query
Showing below up to 51 results in range #1 to #51.
| Name | Category | Progenitor | Type | Energy Mechanism | Emission Mechanism | LF Radio Counterpart | HF Radio Counterpart | Microwave Counterpart | THz Counterpart | OIR Counterpart | X ray Counterpart | Gamma ray Counterpart | GW Counterpart | Neutrino Counterpart | References | Comments |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| NS-WD Accretion | Accretion |
NS-WD |
Repeat | Mag. reconnection |
Curv. |
Yes |
-- |
-- |
-- |
-- |
-- |
Yes, but unlikely detectable |
-- |
-- |
URL | None |
| AGN-KBH | AGN |
AGN-KBH Interaction |
Repeat | Maser |
Synch. |
Yes |
-- |
-- |
-- |
Supernova |
-- |
Yes |
Yes |
Yes |
URL | Neutrinos from preceding SN and from collapse to BH. |
| AGN-SS | AGN |
AGN-Strange Star Interaction |
Repeat | Electron oscillation |
-- |
Yes |
-- |
-- |
-- |
Thermal |
-- |
Yes |
Yes |
Yes |
URL | Neutrinos from preceding SN and from collapse to BH. GW from collapse and persistent GWs from SS. |
| Jet-Caviton | AGN |
Jet-Caviton Interaction |
Both | Electron scattering |
Bremsst. |
Yes |
Yes |
-- |
-- |
-- |
-- |
Possible GRB |
Yes |
-- |
URL • URL | Persistent scintillating radio emission. |
| Wandering Beam | AGN |
Wandering Beam |
Repeat | -- |
Synch. |
Yes |
-- |
-- |
-- |
-- |
Yes |
-- |
-- |
-- |
URL | None |
| NS to BH (DM-Induced) | Collapse |
NS to BH |
Single | Mag. reconnection |
Curv. |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
Yes |
-- |
URL | None |
| NS to KNBH | Collapse |
NS to KNBH |
Single | Mag. reconnection |
Curv. |
Yes |
-- |
-- |
-- |
-- |
Possible afterglow |
Possible GRB |
Yes |
-- |
URL • URL • URL | Possible X-ray afterglow and a short/long GRB created in NS birth prior to the FRB. |
| NS to Quark Star | Collapse |
NS to Quark Star |
Single | β-decay |
Synch. |
Yes |
-- |
-- |
-- |
-- |
Yes |
Yes |
Yes |
-- |
URL | The burst is predicted to be several seconds, explainable if the de-dispersion process that stacks f |
| SS Crust | Collapse |
Strange Star Crust |
Single | Mag. reconnection |
Curv. |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
Yes |
-- |
URL | None |
| Axion Cloud and BH | Collision / Interaction |
Superradiant Axion Cloud and BH |
Repeat | Laser |
Synch. |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
Yes |
-- |
URL | Observational counterparts could be associated with electron-positron annihilation and/or positroniu |
| Axion Minicluster and NS | Collision / Interaction |
Axion Minicluster and NS |
Single | Maser |
Synch. |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL | None |
| Axion Quark Nugget and NS | Collision / Interaction |
Axion Quark Nugget and NS |
Repeat | Mag. reconnection |
Curv. |
Yes |
Possible |
Possible |
-- |
-- |
-- |
-- |
-- |
-- |
URL | None |
| Axion Star and BH | Collision / Interaction |
Axion Star and BH |
Repeat | Electron oscillation |
-- |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL | None |
| Axion Star and NS | Collision / Interaction |
Axion Star and NS |
Single | Electron oscillation |
Coherent dipole radiations |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL • URL • URL • URL • URL | None |
| NS and Primordial BH | Collision / Interaction |
NS and Primordial BH |
Both | Mag. reconnection |
-- |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
Yes |
-- |
URL | None |
| Small Body and Pulsar | Collision / Interaction |
Small Body and Pulsar |
Single | Maser |
Synch. |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL | None |
| NS and Asteroid Belt | Collision/ Interaction |
NS and Asteroid Belt |
Repeat | Electron stripping |
Curv. |
Yes |
-- |
-- |
-- |
-- |
-- |
Yes |
-- |
-- |
URL • URL | None |
| NS and Asteroids/Comets | Collision/ Interaction |
NS and Asteroids/ Comets |
Single | Mag. reconnection |
Curv. |
Yes |
-- |
-- |
-- |
-- |
Yes (probably too faint to detect) |
Yes (probably too faint to detect) |
-- |
-- |
URL | None |
| Pulsar-BH Interaction | Interaction |
Pulsar-BH |
Single | -- |
-- |
Yes |
? |
-- |
-- |
-- |
-- |
-- |
Yes |
-- |
URL | |
| Annihilating Mini BHs | Inviable |
Annihilating Mini BHs |
Single | N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
URL | None |
| Stellar Coronae | Inviable |
Stellar Corona |
Both | N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
N/A |
URL • URL | None |
| KNBH-BH (Inspiral) | Merger |
KNBH-BH |
Single | Mag. flux change |
Curv. |
Yes |
Afterglow |
-- |
-- |
-- |
Yes |
sGRB |
Yes |
-- |
URL | Unlikely to account for full FRB population. |
| KNBH-BH (Magneto. Collapse) | Merger |
KNBH-BH |
Single | Mag. reconnection |
Curv. |
Yes |
Afterglow |
-- |
-- |
-- |
-- |
Afterglow |
Yes |
-- |
URL | Can only account for a sub-population of FRBs. |
| NS-BH Merger | Merger |
NS-BH |
Single | BH battery |
-- |
-- |
-- |
-- |
-- |
-- |
Yes |
Yes |
Yes |
-- |
URL | None |
| NS-NS Merger (Mag. Braking) | Merger |
NS-NS |
Single | Mag. braking |
-- |
Yes |
Yes |
-- |
-- |
Kilonova |
Afterglow |
sGRB |
Yes |
-- |
URL | |
| NS-NS Merger (Mag. Flux Change) | Merger |
NS-NS |
Both | Mag. flux change |
-- |
Yes |
Yes |
-- |
-- |
Kilonova |
Afterglow |
sGRB |
Yes |
-- |
URL | In dense stellar clusters |
| NS-NS Merger (Mag. Reconnection) | Merger |
NS-NS |
Both | Mag. reconnection |
Curv. |
Yes (excl. self absorption) |
Yes |
? |
? |
Kilonova |
Afterglow |
sGRB |
Yes |
-- |
URL | None |
| NS-WD Merger | Merger |
NS-WD |
Single | Mag. reconnection |
Curv. |
Yes |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL | |
| WD-BH Merger | Merger |
WD-BH |
Single | Maser |
Synch. |
-- |
-- |
-- |
-- |
-- |
Yes (transient accretion disk) |
-- |
-- |
-- |
URL | None |
| WD-WD Merger | Merger |
WD-WD |
Single | Mag. reconnection |
Curv. |
Yes |
-- |
-- |
-- |
Supernova |
Afterglow |
-- |
-- |
-- |
URL | -- |
| Young Magnetars | Merger/Collapse |
Magnetars Born in BNS Mergers and WD Col |
Repeat | Maser |
Synch. |
Yes |
Afterglow |
-- |
-- |
Possible SN |
Afterglow |
sGRB |
Yes |
-- |
URL | Same mechanisms as flares, but magnetars born in mergers or collapse as opposed in to SLSNe or LGRBs |
| Alien Light Sails | Other |
Alien Light Sails |
Repeat | Artificial transmitter |
-- |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL | Highly speculative. |
| DSR in Galaxies | Other |
Dicke's Superradiance in Galaxies |
Both | Dicke's Superradiance |
Spectral line |
Yes |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL • URL | -- |
| Magnetars with Low Magnetospheric Twist | Other |
Magnetars with Low Magnetospheric Twist |
Repeat | Mag. reconnection |
Pulsar-like |
Yes |
--- |
Maybe |
Maybe |
Maybe |
Maybe |
Unlikely detectable |
--- |
--- |
URL • URL | Unlikely to form in Galactic magnetars. |
| Neutral Cosmic Strings | Other |
Neutral Cosmic Strings |
Single | Cusp decay |
-- |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL | None |
| NS Combing | Other |
NS Combing |
Both | Various |
Mag. reconnection |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL • URL | The model can apply to a variety of events, and thus counterparts will depend on the scenario. |
| Pulsar Lightning | Other |
Pulsar Lightning |
Repeat | Electrostatic |
Curv. |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL | None |
| RDM Stars | Other |
RDM Star |
Both | Stimulated emission |
Synch. |
--- |
--- |
--- |
--- |
--- |
--- |
--- |
--- |
--- |
URL • URL | Repeaters are possible if multiple asteroids collide with the star |
| Starquakes | Other |
Starquakes |
Repeat | Mag. reconnection |
Curv. |
Yes |
-- |
-- |
-- |
Possible |
Possible |
Yes |
Yes, but unlikely detectable |
-- |
URL • URL | None |
| Superconducting Cosmic Strings | Other |
Superconducting Cosmic Strings |
Single | Cusp decay |
-- |
Yes |
-- |
-- |
-- |
-- |
-- |
GRB |
Yes |
Yes |
URL • URL • URL | High energy cosmic rays are also expected. |
| Tiny EM Explosions | Other |
Tiny EM Explosions |
Both | Thin shell interactions |
Curv. |
Yes |
Yes |
-- |
-- |
-- |
-- |
Unlikely observable |
-- |
-- |
URL • URL | None |
| Variable Stars | Other |
Variable Stars |
Repeat | Undulator |
Synch. |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL | None |
| Wandering Pulsar | Other |
Wandering Pulsar Beams |
Repeat | -- |
-- |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL | Any counterparts will be associated with the pulsar, but are not specified. |
| White Holes | Other |
White Holes |
Single | -- |
-- |
Yes |
-- |
-- |
-- |
Yes |
-- |
Yes |
-- |
-- |
URL • URL | None |
| Decelerating Blast Waves | Shock Interaction |
Magnetar |
Repeat | Thin shell |
Synch. Maser |
Yes |
Yes |
-- |
-- |
Possible, Prompt |
Prompt |
Prompt |
No |
No |
URL | None |
| NS-SN Interaction | Shock Interaction |
NS-SN Interaction |
Single | Mag. reconnection |
-- |
Yes |
-- |
-- |
-- |
Supernova |
-- |
possible GRB (low flux) |
-- |
-- |
URL | |
| MWN Shock (Clustered Flares) | SNR (Magnetars) |
MWN Shock (Clustered Flares) |
Repeat | Maser |
Synch. |
Yes |
Afterglow |
-- |
-- |
Possible bright optical |
Yes but ~100 years later |
Low energy gamma-rays, sGRB if jet aligned |
Yes |
-- |
URL | FRB 121102 may by unlikely in this scenario. |
| MWN Shock (Single Flare) | SNR (Magnetars) |
MWD Shock (Single Flare) |
Single | Maser |
Synch. |
Yes |
Afterglow |
-- |
-- |
Maybe |
-- |
Low energy gamma-rays, sGRB if jet aligned |
Yes |
-- |
URL • URL • URL | None |
| Giant Pulses | SNR (Pulsars) |
Giant Pulses |
Repeat | -- |
Synch. |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL • URL • URL | Rapid flux decay expected to be observed within a few years. |
| Pulsar Schwinger Pairs | SNR (Pulsars) |
Pulsar Schwinger Pairs |
Single | Schwinger |
Curv. |
Yes |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
-- |
URL | None |
| Pulsar Wind Bubble | SNR (Pulsars) |
Pulsar Wind Bubble (NS and MWD) |
Single | -- |
Synch. |
Yes |
-- |
-- |
-- |
-- |
Yes |
-- |
-- |
-- |
URL | None |
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