13 questions · 7 sources · 0 syntheses
Neutron Stars and Pulsars
Ultra-dense stellar remnants and their rotating beacons.
Source-derived questions
Questions extracted from the papers in this topic, excluding the curated questions above.
- How did Aleksander Wolszczan detect planets orbiting a pulsar using radio pulse timing?
- How did Riccardo Giacconi's X-ray telescopes change what astronomers could see in the cosmos?
- How did Russell Hulse first notice that PSR B1913+16 was actually a binary pulsar rather than an ordinary one?
- How might the planets around PSR B1257+12 have survived or formed after the supernova?
- What has FAST discovered about pulsars since beginning operations?
- What is a neutron star, and how does its spin produce such a precisely timed radio pulse?
- What later scientific discoveries did the Lovell Telescope contribute to beyond tracking early space missions?
- What signal in the data first tipped off Antony Hewish's team to the existence of pulsars?
- What was unusual about the radio pulse Jocelyn Bell noticed in the chart-recorder data in August 1967?
- Why did Bell's team briefly nickname the signal 'LGM-1' before settling on a natural explanation?
- Why did Jocelyn Bell Burnell, who first spotted the pulsar signal, not share in the 1974 Nobel Prize?
- Why did the 1974 Nobel Prize for the pulsar discovery go to Bell's supervisor rather than to her?