Zapis dokaza metode
Rotation Curve Analysis
Galaxy rotation curve analysis is the technique of measuring how orbital velocities change with distance from the center of a galaxy. Pioneered by Vera Rubin and W. Kent Ford Jr. in 1970, rotation curves revealed one of astronomy's great mysteries: galaxies rotate too fast to be held together by their visible stars alone, providing direct evidence for dark matter.
Izvorni zapis
Citati kopirani doslovno iz izvornog zapisa metode. Ne impliciraju nikakvu provjeru na razini tvrdnje.
Galaxy Rotation Curve Analysis for Dark Matter Detection
Taksonomski zapis metode · process-pipeline / astronomy
- Vera C. Rubin & W. Kent Ford Jr. (1970). Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission Regions. Astrophysical Journal, 159, 379-403. · DOI 10.1086/150317
- Flores, R. A., & Primack, J. R. (1994). Structure and dynamics of galactic dark matter halos. Astrophysical Journal Letters, 427(1), L1-L4. · URL
- Sofue, Y., Tutui, Y., Honma, M., et al. (2001). Central and dark matter rotation curves of spiral galaxies. Astrophysical Journal, 547(2), 712-726. · URL
Uređene tvrdnje
Tvrdnje pohranjene u knjigu dokaza, svaka s vlastitom procjenom.
Nema uređenih tvrdnji
Ovaj prikaz ne izmišlja procjenu tvrdnje kada knjiga dokaza nema nijednu.
Povezane metode
Generirano iz grafa metode i prikazano kao strojno predložene relacije — ne implicira se nikakva tvrdnja dokaza.