Best fit model of the Radcliffe Wave
Harvard Dataverse (Africa Rice Center, Bioversity International, CCAFS, CIAT, IFPRI, IRRI and WorldFish)
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Title |
Best fit model of the Radcliffe Wave
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Identifier |
https://doi.org/10.7910/DVN/F98QHY
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Creator |
Konietzka, Ralf
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Publisher |
Harvard Dataverse
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Description |
Tab-separated ASCII machine readable table of the best fit model in Konietzka et al. 2024. The best fit model was derived by applying the model described in Konietzka et al. 2024 to the spatial and kinematic molecular cloud and stellar cluster observations. Data columns are as follows: (1) x: Heliocentric Galactic Cartesian x position (pc) (2) y: Heliocentric Galactic Cartesian y position (pc) (3) z: Heliocentric Galactic Cartesian z position (pc) (4) vz: motion along the Heliocentric Galactic Cartesian z direction (km/s) |
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Subject |
Astronomy and Astrophysics
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Date |
2024-03-08
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Contributor |
Konietzka, Ralf
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