Color-difference photometry of the Crab Nebula pulsar and the rotating relativistic vector model

Details Color-difference photometry of the Crab Nebula pulsar and the rotating relativistic vector model Color-difference photometry of the Crab Nebula pulsar and the rotating relativistic vector model

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...194..725c&link_type=abstract

Astrophysical Journal, vol. 194, Dec. 15, 1974, pt. 1, p. 725-731.

Astronomy and Astrophysics

Astrophysics

13

Astronomical Models, Crab Nebula, Light Curve, Pulsars, Relativistic Theory, Luminous Intensity, Mathematical Models, Tables (Data), Ubv Spectra, Vector Analysis

Scientific paper

Light curves of the Crab Nebula pulsar in U and V are given, as are normalized difference curves for the main and secondary pulses. The ratios of total intensity for main to secondary are: 1.866 for U, and 1.916 for V. The intensity difference curve for the secondary pulse is fitted by the rotating relativistic vector model. Timing errors prevent a fit for the main pulse.

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