LYNGA:7 - Relative Phases of the X-Ray and Gamma-Ray Pulses

Details LYNGA:7 - Relative Phases of the X-Ray and Gamma-Ray Pulses LYNGA:7 - Relative Phases of the X-Ray and Gamma-Ray Pulses

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...273..421b&link_type=abstract

Astronomy and Astrophysics, Vol.273, NO. 2/JUNII, P. 421, 1993

Astronomy and Astrophysics

Astrophysics

14

Pulsars: Individual (Geminga), X-Rays: Stars, Stars: Neutron, Γ-Rays: 1E 0630+178 Observations

Scientific paper

Measurements of the relative phases of pulses in separate energy bands provide important information about the geometry of pulsars' emission regions. The lack of pulsars detected in different wave bands has hampered this approach in the past. Here we present an analysis of ROSAT data on Geminga and give the phase relationship between the X-ray and MeV-GeV lightcurves. The X-ray emission is sinusoidal and maximizes just before the second γ-ray peak.

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