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Showing below up to 20 results in range #11 to #30.

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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 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.

Wandering Pulsar

Other

Wandering Pulsar Beams

Repeat

--

--

Yes

--

--

--

--

--

--

--

--

URL

Any counterparts will be associated with the pulsar, but are not specified.

Superconducting Cosmic Strings

Other

Superconducting Cosmic Strings

Single

Cusp decay

--

Yes

--

--

--

--

--

GRB
if jet aligned

Yes

Yes

URL URL URL

High energy cosmic rays are also expected.

Variable Stars

Other

Variable Stars

Repeat

Undulator

Synch.

Yes

--

--

--

--

--

--

--

--

URL

None

DSR in Galaxies

Other

Dicke's Superradiance in Galaxies

Both

Dicke's Superradiance

Spectral line

Yes

Yes

--

--

--

--

--

--

--

URL URL

--

Neutral Cosmic Strings

Other

Neutral Cosmic Strings

Single

Cusp decay

--

Yes

--

--

--

--

--

--

--

--

URL

None

Starquakes

Other

Starquakes

Repeat

Mag. reconnection

Curv.

Yes

--

--

--

Possible

Possible

Yes
if pulsar jet aligned

Yes, but unlikely detectable

--

URL URL

None

White Holes

Other

White Holes

Single

--

--

Yes

--

--

--

Yes

--

Yes

--

--

URL URL

None

RDM Stars

Other

RDM Star

Both

Stimulated emission

Synch.

---

---

---

---

---

---

---

---

---

URL URL

Repeaters are possible if multiple asteroids collide with the star

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.

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

WD-BH Merger

Merger

WD-BH

Single

Maser

Synch.

--

--

--

--

--

Yes (transient accretion disk)

--

--

--

URL

None

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
if jet aligned

Yes

--

URL
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.

KNBH-BH (Inspiral)

Merger

KNBH-BH

Single

Mag. flux change

Curv.

Yes

Afterglow

--

--

--

Yes

sGRB
if jet aligned

Yes

--

URL

Unlikely to account for full FRB population.

WD-WD Merger

Merger

WD-WD

Single

Mag. reconnection

Curv.

Yes

--

--

--

Supernova

Afterglow

--

--

--

URL

--

NS-NS Merger (Mag. Flux Change)

Merger

NS-NS

Both

Mag. flux change

--

Yes

Yes

--

--

Kilonova

Afterglow

sGRB
if jet aligned

Yes

--

URL

In dense stellar clusters

NS-WD Merger

Merger

NS-WD

Single

Mag. reconnection

Curv.

Yes

Yes

--

--

--

--

--

--

--

URL
NS-NS Merger (Mag. Reconnection)

Merger

NS-NS

Both

Mag. reconnection

Curv.

Yes (excl. self absorption)

Yes

?

?

Kilonova

Afterglow

sGRB
if jet aligned

Yes

--

URL

None

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