Exam 15: Star Formation and the Interstellar Medium

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What happens as a protostar contracts?

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What is the most likely explanation for the dark area in the image below? What is the most likely explanation for the dark area in the image below?

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The red emission in the photo below is due to: The red emission in the photo below is due to:

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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.

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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.

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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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Why do many stars form from a single molecular cloud?

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Stars forming in molecular clouds tend to form first in the low-density periphery.

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Magnetic fields inside a molecular cloud act to:

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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. 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. 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.

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Interstellar clouds are:

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As a protostar evolves, its temperature:

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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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