21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 16, Problem 3QP
To determine

The situation of star when it follows a horizontal path across the H-R diagram.

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The total mass of a binary system can be calculated from   a. the ratio of the angular separation from the center of mass of each of the stars.   b. the distance to the binary and its radial velocity.   c. the semi major axis and period of the orbit.   d. the radial velocities of the two stars.   e. the time required for the small star to eclipse the larger star.
The hydrogen lines in spectral type A stars   a. are most narrow for supergiants.   b. are most narrow for main-sequence stars.   c. cannot be used to estimate the luminosity of the star.   d. are very weak and difficult to see.   e. are useful in determining the apparent magnitude of the star.
The gas and dust cocoon surrounding young stars   a. is blown away when the young stellar surface heats up and becomes more luminous.   b. remains surrounding the young star throughout its adult life.   c. eventually collapses onto the star, increasing its mass and luminosity.   d. evaporates gradually over the lifetime of the star.   e. expands as the star’s luminosity increases eventually reaching a distance far enough that it condenses to form comets.
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