Exam 9: The Formation and Structure of Stars

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There is a main-sequence mass-luminosity relation because

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What is the lifetime of a 10-solar-mass star on the main sequence?

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Which of the following is NOT evidence of the existence of an interstellar medium?

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ZAMS is an acronym for ______________________________.

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  The above visual wavelength image of the Trapezium cluster shows _________. The above visual wavelength image of the Trapezium cluster shows _________.

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More massive stars have more weight to support, so these stars are more luminous.

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What is the difference between the proton-proton chain and the CNO cycle?

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The average star spends ________ of its lifetime on the main sequence.

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The interstellar medium is made of ___ % dust and ___ % gas.

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Due to the dust in the interstellar medium, a distant star will appear to an observer on Earth to be

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____________________ is the resistance of a gas to the flow of radiation.

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The dust in the interstellar medium can make distant stars look redder than they really are.

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YSOs are in hydrostatic equilibrium.

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The central cores of which type of star is the lowest temperature?

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  In the Herbig-Haro object shown above, the Herbig-Haro is the ___________. In the Herbig-Haro object shown above, the Herbig-Haro is the ___________.

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The pressure of a gas depends on the temperature and density of the gas.

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Why are massive stars more luminous than low mass stars? That is, why is there a mass-luminosity relation?

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  The above reactions are of the ___________________. The above reactions are of the ___________________.

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Ionization from the ____________________ star in the Orion nebula makes it ____________________ brightly.

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What is the correct fraction of dust to gas in the interstellar medium?

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