Scientific American - USA (2020-12)

(Antfer) #1

Mass of star (relative to the sun)


8–10× Electron-capture supernova Neutron star

10–20× Type-II core-collapse supernova Neutron star

20–40× Type-II core-collapse supernova Black hole

40–100× Type-Ibc core-collapse supernova Black hole

Greater than 260× Black hole

100–260× Pair-instability supernova Nothing

Death progression Corpse (remnant)

?

Dense shell
of gas
and dust made
of carbon
and oxygen

Star

Gamma-ray burst
(black hole launches a fast jet)
or dirty fireball (black hole launches a slow jet)

Rapidly spinning black hole

Stellar remnant material

Jet

Superluminous supernova
(neutron star launches a wind)

Neutron star with strong
magnetic field (magnetar)

Wind

Stellar remnant/
material

Slow jet launched by
a black hole
or maybe a magnetar
driving a wind

AT2018cow

A dense torus of
gas and dust that
presumably used
to be part of
the star and
was recently shed

Jets stifled inside
recently shed material

Jet

Jet cocoon

Spinning
black hole

Neutron star
(likely)

SN2018gep Explosion debris hits shell

B ● ODDITY: ENGINE-DRIVEN EXPLOSIONS
3ometimes it seems that the corpse of a dead star€a newly created
neutron star or black hole€remains active and forms an engine
that launches a powerful ¦et or wind. This probably happens when
the starÝs core is rotating extremely quickly at the time of collapse.
$aybe the star was spinning fast to begin with or gained speed
through an interaction with a binary companion. Examples of
engine-driven explosions are shown here
Êcircled in green, orange and yellowË.
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