Presentation from 28th March 2017 to Brighton Astro group. Slideshare removes embedded videos, so two in here are the following:
https://www.youtube.com/watch?v=e-P5IFTqB98&t=18s
https://www.youtube.com/watch?v=NhOVDDiSvMM
2. • Proposed by Walter Baade & Fritz Zwicky in
1934
• Jocelyn Bell Burnell and Antony Hewish in
1967 – LGM-1
• Now more than 2000 discovered
HISTORY OF DISCOVERY
6. SMALLER STARS (LIKE OUR SUN)
( Don’t worry, we have around 5
billions years left yet … )
8. ALL ABOUT MASS OF CORE REMNANT
< 1.4 Solar Masses = White dwarf
1.4 - ~3 Solar Masses = Neutron star
> 3 Solar Masses = Black hole
9. MASS OF ORIGINAL STAR
< 10 Solar masses = White dwarf
10 – 29 Solar masses = Neutron star
> 29 Solar masses = Black hole
10. SOME OTHER SCENARIOS….
• Some stars may just vanish to black hole instantly
• Some huge stars blow up entirely, leaving NOTHING
• Some may form Quark Stars
11. NEUTRON STAR
• All empty space of atoms squeezed away
• Density of an atom core
• Tight structure of neutrons
• Matchbox of material = 13m tonnes
• Cube of Earth 135m square
18. SPIN RATE
Spin Up -
Angular
momentum
transferred
from accreting
material
19. SPIN RATE
• MSP – fastest 700x / second!
• 24% the speed of light!
• Upper limit 1500 x ?
• Slow as they age and stop accreting
• Slowest yet found – 6.7 hrs
20. TYPES OF NEUTRON STARS
• “Quiet” neutron stars, non emitting
• Binary pair
• Pulsars
• Magnetars
23. PULSARS
• Highly magnetic, emit beams of energy
• Very, very precise spin rates
• Spinning from every few seconds, to
700 x per second
• 23% of the speed of light!
• Potential uses as deep space GPS signals
• Pulsar clock built in Gdańsk
28. MAGNETARS
• Even more powerful magnetic field
• Rotate more slowly ( 1 – 10 seconds )
• Strong bursts of x-rays and gamma rays
• Magnetic fields tend to decay after 10,000 years
• 30m estimated inactive magnetars in Milky Way
30. HOW COMMON?
• Estimated at 1bn in Milky Way
• Only 2000 found so far
• Many are old and have slowed, lost energy
• Nearest to us ~280 light years away