Expected number of blue-shifts and red-shifts of ejected sources.
Doppler effect in quasar red-shifts and theoretical expected number of blue-shifts and red-shifts of ejected sources
STELLAR DOPPLER SHIFT↗
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The gravitational red shift
Relativistic red shift effect and its measurement by hydrogen maser clock
Eby, P.↗
Doppler interpretation of quasar red shifts.
Quasi-stellar sources as local objects moving with velocities close to speed of light, noting transverse Doppler effect leads to expectation of fewer blue shifts than red shifts
DOPPLER EFFECT↗
Red shift of auroral hydrogen profiles.
Red shift of magnetic zenith hydrogen line profiles and role of injection pitch-angle distribution of auroral protons
GEOMAGNETIC FIELD↗
Relation between the red-shifts of quasi- stellar objects and their radio and optical magnitudes.
Red shifts of quasi-stellar objects and relation to radio and optical magnitudes, concluding that red shifts have no relation to distance
QUASI-STELLAR RADIO SOURCE /QSO/↗
Evidence for a correlation between the position and red-shift of quasars.
Correlation between position and red shift of quasars indicating anisotropic universe or galactic origin of quasars
ASTRONOMICAL SPECTRUM↗
The second-order gravitational red shift
The direct measurement of the nonlinear term of the gravitational field equations by using very stable clocks is discussed along with measuring the perhelion advance of a planet or satellite. These are considered measurements of the second-order gravitational red shift. The exact expression for the frequency shift of light in a gravitational field is derived. Other topics discussed include: The Doppler-cancelling technique; the second-order red shift in a spherically symmetric gravitational field; finite signal transit time; and the reality and interpretation of coordinates in the second-order red shift experiment.
Jaffe, J.↗
An orbiting clock experiment to determine the gravitational red shift
Orbiting clock experiment for measuring gravitational red shift of earth by comparing ground based and satellite-borne hydrogen maser clocks
Kleppner, D.↗
Dependence of the optical continuous spectrum of quasars on their red-shift
Dependence of optical continuous spectrum of quasi-stellar sources on red shift
OPTICAL SPECTRUM↗
Relation between the red-shifts of quasi- stellar objects and their radio magnitudes.
Quasi-stellar object red shift correlation with radio magnitude
RED SHIFT↗
Red-shift arising from light passage in a magnetic field Semiannual report
Photon-photon scattering model for red shift of light passing through magnetic field
RED SHIFT↗
A tentative explanation of cosmological red shift
The authors suggest a possible alternative explanation of cosmological red shift. They consider that there exists a background field in the universe, and that light (the photon) has an extremely weak interaction with this background, and as result, experiences an energy loss. By analogy with damped oscillations, the authors introduce a dumping term with the first derivative with respect to time in the wave equation. The solution yields a linearly reduced frequency of the light with travel distance. The purpose of this exercise is to demonstrate how a simple alternative interpretation of the Hubble relation can be generated.
Chang, T.↗
GRO: Red-shifted electron-positron annihilation gamma-rays from radiopulsars
Reported red-shifted e(+) + e(-) yields gamma + gamma 511 keV gamma-rays from the Crab pulsar would, if ultimately confirmed, provide crucial clues about the structure of the powerful magnetospheric accelerator in that rapidly spinning gamma-ray pulsar. In an attempt to understand the origin of this component of the Crab pulsar's emission, we try to account for the following: (1) a flow of approximately 10 exp 40 e(+/-)/s into near the surface of the neutron star; (2) a relatively narrow annihilation line implying that the annihilating e(+/-) pairs probably had a velocity (along vector B) less than or approximately = 10(exp -1)c; and (3) a tentative light curve suggesting a doubly peaked structure different from that of the rest of the Crab pulsar's nonthermal radiation.
Ruderman, Malvin↗
The Red-Shift Magnitude Relation and Observational Data
Red shift-magnitude relation for universe model and observational data
Sherman, Windsor L.↗
A Doppler-Cancellation Technique for Determining the Altitude Dependence of Gravitational Red Shift in an Earth Satellite
A cancellation technique permits measurement of the frequency of a source moving relative to an observer without the obscuring effect of first-order Doppler shifts. The application of this method to a gravitational red shift experiment involving the use of an earth satellite containing a highly stable oscillator is described. The rapidity with which a measurement can be made permits the taking of data at various altitudes in a given elliptical orbit. Tropospheric and ionospheric effects upon the accuracy of results are estimated.
Badessa, R. S.↗
On the possibility of measuring the gravitational red shift using a synchronous satellite, a laser and a Fabry-Perot interferometer.
Gravitational red shift measurement using synchronous satellite, argon laser and Fabry- Perot interferometer
Ransford, G.↗
Red-shifts of quasi-stellar objects and related extragalactic systems.
Quasi-stellar and related objects emission and absorption red shifts tabulation suggesting absorption lines origin
Burbidge, E. M.↗
An X-ray red-shift test for clusters of galaxies up to Z greater than or equal to 1
Correlated measurements of red-shifted iron line emission and apparent surface brightness are suggested for unambiguously defining intrinsic X-ray characteristics for clusters of galaxies up to z greater than or equal to 1. If some of the weak unidentified high galactic latitude X-ray sources are clusters at z approximately 1-3, then such correlated measurements should be feasible witin the complement of instruments aboard the HEAO-B orbiting X-ray telescope observatory. In addition, those clusters at z less than 1 would require spectral data from broader bandwidth experiments, such as the all-sky survey to be provided by the proportional counters aboard the first mission of the High Energy Astronomy Observatory (HEAO-A).
Boldt, E. A.↗