Foundations of Astronomy (MindTap Course List)
Foundations of Astronomy (MindTap Course List)
14th Edition
ISBN: 9781337399920
Author: Michael A. Seeds, Dana Backman
Publisher: Cengage Learning
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Chapter 12, Problem 14P
To determine

The distance of the Delta Cephei and find the magnitude-distance of Delta Cephei.

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result, the -1 from a T Tauri star, estimate the mass density of the wind at a distance of 100 AU from the star. (Hint: Refer to Example 11.2.1.) Compare your answer with the density of the giant molecular cloud agpalain Example 12.2.1. 12.19 Assuming a mass loss rate of 10-7 Mo yr¹ and a stellar wind velocity of 80 km s -niem-1299 ear
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12.1 In a certain part of the North American Nebula, the amount of interstellar extinction in the visual wavelength band is 1.1 magnitudes. The thickness of the nebula is estimated to be 20 pc, and it is located 700 pc from Earth. Suppose that a B spectral class main-sequence star is observed in the direction of the nebula and that the absolute visual magnitude of the star is known to be My = -1.1 from spectroscopic data. Neglect any other sources of extinction between the observer and the nebula. (a) Find the apparent visual magnitude of the star if it is lying just in front of the nebula. (b) Find the apparent visual magnitude of the star if it is lying just behind the nebula. Problems 443 (c) Without taking the existence of the nebula into consideration, based on its apparent mag- nitude, how far away does the star in part (b) appear to be? What would be the percentage error in determining the distance if interstellar extinction were neglected?
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