TRANSPORT OF THE FIRST ROCKS OF THE SOLAR SYSTEM BY X-WINDS
It has been suggested that chondrules and calcium-aluminum-rich inclusions (CAIs) were formed at the inner edge of the protoplanetary disk and then entrained in magnetocentrifugal X-winds. We study trajectories of such solid bodies with the consideration of the central star gravity, the protoplaneta...
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| Format: | Article |
| Language: | English |
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Institute of Physics/American Astronomical Society,
2015-03-05T15:31:56Z.
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| Online Access: | Get fulltext |