Abstract
We report new results obtained from the EXOSAT AO- 1 observation of the intermediate polar V1223 Sgr. The detection of a 12.4 minute period in the medium energy X-ray flux with an associated hardness ratio variation has been previously reported in Osborne et al. (1984a). Further work has revealed: a narrow dip at the phase zero in the folded medium energy light curve; ~ 30% modulation in the low energy X-ray (3000 Lexan) flux; a count rate ratio from 3 filters which allow the presence of a bright low temperature blackbody component (kT = .05 - .40 KeV); and a phase resolved ME spectrum which must have two or more components when the source is bright. New optical ephemerides show that the X-ray and optical pulses are in phase at an orbital phase of φ= 0.31.
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© 1985 D. Reidel Publishing Company
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Osborne, J.P., Rosen, R., Mason, K.O., Beuermann, K. (1985). New Exosat Results from the Intermediate Polar V1223 SGR. In: Peacock, A. (eds) X-Ray Astronomy in the Exosat Era. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5448-9_18
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DOI: https://doi.org/10.1007/978-94-009-5448-9_18
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-8906-7
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