What are potential solutions to the missing satellites problem (i.e. solutions that solve the problem without discarding ACDM)? (Choose 3). O If simulations include a Galactic potential, fewer dark matter halos survive. Many low-mass galaxies exist, but are not bright enough to be seen by current telescopes. O Low mass galaxies merge into large galaxies and become part of their stellar halos. O The number of low mass dark matter halos that form is lower than predictions based on cosmological initial conditions. O lonizing photons from the first stars, galaxies or quasars heat gas until the pressure is too high to collapse into the smallest dark matter hale O Dwarf galaxies stream out of voids and into clusters and superclusters where they merge into larger galaxies.

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What are potential solutions to the missing satellites problem (i.e. solutions that solve the problem without discarding ACDM)? (Choose 3).
O If simulations include a Galactic potential, fewer dark matter halos survive.
Many low-mass galaxies exist, but are not bright enough to be seen by current telescopes.
O Low mass galaxies merge into large galaxies and become part of their stellar halos.
O The number of low mass dark matter halos that form is lower than predictions based on cosmological initial conditions.
O lonizing photons from the first stars, galaxies or quasars heat gas until the pressure is too high to collapse into the smallest dark matter halos.
O Dwarf galaxies stream out of voids and into clusters and superclusters where they merge into larger galaxies.
Transcribed Image Text:What are potential solutions to the missing satellites problem (i.e. solutions that solve the problem without discarding ACDM)? (Choose 3). O If simulations include a Galactic potential, fewer dark matter halos survive. Many low-mass galaxies exist, but are not bright enough to be seen by current telescopes. O Low mass galaxies merge into large galaxies and become part of their stellar halos. O The number of low mass dark matter halos that form is lower than predictions based on cosmological initial conditions. O lonizing photons from the first stars, galaxies or quasars heat gas until the pressure is too high to collapse into the smallest dark matter halos. O Dwarf galaxies stream out of voids and into clusters and superclusters where they merge into larger galaxies.
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