The redshift of the quasi-stellar radio source 3c 286.
Redshift of quasi-stellar radio source 3C 286 determined by prime-focus photoelectric spectrum scanner, considering emitting elements for various lines
SEARCH · Search NASA
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Redshift of quasi-stellar radio source 3C 286 determined by prime-focus photoelectric spectrum scanner, considering emitting elements for various lines
Redshift of quasi-stellar radio source 3C 279
Variations in optical spectrum of quasi-stellar radio source 3C 345
Absorption lines of quasi-stellar object 3C 191
Red shift relationship with ionization potential for absorption lines in quasi-stellar object 3C 191
Spectral energy distribution of source 3C 446 between August 17 and December 12, 1966
Diameter and position of radio source 3C 132 determined by lunar occultation, confirming identification with red galaxy
Optical variations in radio galaxy 3C 371 from photoelectric spectrum analysis, discussing quasi- stellar sources
Optical polarization of 3C 273 on various nights noting mean polarization
Fringe amplitude measurement of 3C 273 using interferometer at 18 cm wavelength
Gamma ray flux limits from 3C 273 and M 87 using balloon data
Tests of bending strength on full scale model of Atlas LV-3C booster
Extragalactic objects 3C 273 NGC 5128 and M87 X ray emission detection, using proportional counters on Aerobee 150 rocket
Computer programs to calculate and analyze pion and nucleon interaction within prescribed medium referred to as PROPER 3C Transport Code
Strong and weak emission red shifts of N galaxy 3C 390.3 in Balmer lines, indicating nonisothermal source and gas ejection
M87, Cen A NGC 5128 and 3C 273 X ray emission observations in Virgo cluster, using Uhuru satellite