Exam 15: Star Formation and the Interstellar Medium
Exam 1: Why Learn Astronomy92 Questions
Exam 2: Patterns in the Skymotions of Earth96 Questions
Exam 3: Motion of Astronomical Bodies91 Questions
Exam 4: Gravity and Orbits88 Questions
Exam 5: Light87 Questions
Exam 6: The Tools of the Astronomer94 Questions
Exam 7: The Birth and Evolution of Planetary Systems87 Questions
Exam 8: The Terrestrial Planets and Earths Moon99 Questions
Exam 9: Atmospheres of the Terrestrial Planets92 Questions
Exam 10: Worlds of Gas and Liquid the Giant Planets92 Questions
Exam 11: Planetary Adornmentsmoons and Rings93 Questions
Exam 12: Dwarf Planets and Small Solar System Bodies89 Questions
Exam 13: Taking the Measure of Stars88 Questions
Exam 14: Our Starthe Sun88 Questions
Exam 15: Star Formation and the Interstellar Medium89 Questions
Exam 16: Evolution of Low-Mass Stars90 Questions
Exam 17: Evolution of High-Mass Stars90 Questions
Exam 18: Relativity and Black Holes90 Questions
Exam 19: The Expanding Universe90 Questions
Exam 20: Galaxies95 Questions
Exam 21: The Milky Waya Normal Spiral Galaxy96 Questions
Exam 22: Modern Cosmology92 Questions
Exam 23: Large-Scale Structure in the Universe65 Questions
Exam 24: Life61 Questions
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What is the most likely explanation for the dark area in the image below? 
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The entire process of star formation is really just an evolving balance between:
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The interstellar medium is divided up into three different kinds of gas clouds: cold gas at 10 K, warm gas at 8000 K, and hot gas at about 1 million K.
(True/False)
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Molecular hydrogen atoms are found only inside dense clouds where they are shielded from stellar radiation.
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When a molecular cloud fragments and stars form, the least massive stars are the first to form while the most massive stars take longer to form.
(True/False)
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Star formation in a molecular cloud can be slowed by the strength of its magnetic field and turbulence caused by supernovae and stellar winds from massive stars.
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Stars forming in molecular clouds tend to form first in the low-density periphery.
(True/False)
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Because angular momentum must be conserved, as a gas cloud contracts due to gravity it will also:
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A protostar's evolutionary "track" in the H-R diagram traces out:
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A _________ is a failed star that shines primarily because of energy derived from its gravitational collapse rather than nuclear burning.
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Below are three pictures of the disk of the Milky Way, taken in three different wavelength ranges.
Put the three pictures in order from shortest to longest wavelength.
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A protostar is usually in hydrostatic equilibrium as its collapses.
(True/False)
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Describe the general process of how the interstellar medium can create a star.
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Why can we see dust in the interstellar medium better at far-infrared wavelengths than we can at optical wavelengths?
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