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• Hayashi track
  ...osity against temperature, the track is a nearly vertical curve. After a [[protostar]] ends its phase of rapid contraction and becomes a [[T Tauri star]], it is ...quilibrium]], even those that are partially or fully radiative. Newborn [[protostar]]s start out in this zone, but are not in hydrostatic equilibrium and will
  22 KB (3,584 words) - 12:34, 5 February 2018