Exploring the Cosmos - Degree Exam 2013 - Life and Death of Stars (Part 2)
1. Open clusters within the Galaxy
often contain metal-rich stars.
contain about 1 million stars in a sphere of typically 25 parsecs diameter.
are never surrounded by dust clouds.
usually contain only very old stars which have then spread apart.
2. White dwarfs are
about as hot as the Sun but typically smaller.
so hot that IR radiation dominates, but smaller than the Sun.
typically hot enough to be strong X-rays emitters and about the size of the Earth.
cold and tiny compared to the Sun.
3. The crab pulsar is seen to pulse brightly
about once a day.
nearly 30,000 times each second.
about 30 times each second.
only very rarely.
4. Protostars are normally visible in which two bands of the electromagnetic spectrum?
Radio and visible.
UV and gamma.
visible and UV.
IR and x-ray.
5. The helium flash occurs
in the few seconds before a supernova explosion in a 10 solar mass star.
when fusion begins in a proto-star of about 1 solar mass.
when a 1 solar mass black hole forms from a white dwarf.
in a star of 1 solar mass near the end of the main sequence stage.
6. Pulsars are
too hard to detect to be able to make any clear statements about them.
never observed as gamma-ray objects.
seen in all the main observing bands within the EM spectrum.
always observed as optical objects.
7. Supermassive stars
are the usual precursors of white dwarfs.
are too large to form black holes.
form iron cores in the final stages of their development
live longer than all other types of star, as they have a greater store of fuel.
8. Type II supernovae
are rare but exceedingly bright night-sky objects lasting many years.
are thought to be due to gravitational collapse of a white dwarf.
typically show hydrogen lines in their spectra.
are well-recognised standard candles.
9. Sirius B is
a star slightly heavier than Sirius A that causes Sirius A to wobble.
the "dog star"
a black hole that is difficult to observe because it is so close to Sirius a which is a very bright star.
a white dwarf close to Sirius A.
10. Neutron degeneracy
determines the size of black holes smaller than 3 solar masses.
prevents neutron stars from collapsing to form black holes.
prevents white dwarfs from collapsing to form neutron stars.
affects how neutrons react within the proton-proton chain.
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