Neutron Stars Are Expected to Spin Rapidly Because

question 13

Multiple Choice

Neutron stars are expected to spin rapidly because

• A)they conserved angular momentum when they collapsed.
• B)they have high orbital velocities.
• C)they have high densities.
• D)they have high temperatures.
• E)the energy from the supernova explosion that formed them made them spin faster.

Understand the concept of cross-price elasticity of demand.

Learn how the price elasticity of demand varies with the type and characteristics of goods.

Know the difference in price elasticity between substitutes and complementary goods.

Learn the impact of price changes on the demand for related goods (complements and substitutes).

---

Definitions:

Depreciation Method

A systematic approach to allocating the cost of a tangible asset over its useful life.

Fixed Assets

Fixed assets are long-term tangible assets intended for use in the production or supply of goods or services, not easily converted to cash within a year.

Residual Value

The estimated salvage value of an asset after its useful life is over.

Fully Depreciated

Describes an asset that has reached the end of its useful life, with its cost fully expensed against income over its defined accounting period.