Scattering/absorption dips in 4U1755-33 - Evidence for disc oscillations?

Details Scattering/absorption dips in 4U1755-33 - Evidence for disc oscillations? Scattering/absorption dips in 4U1755-33 - Evidence for disc oscillations?

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...138l..15f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 138, no. 2, Sept. 1984, p. L15, L16.

Astronomy and Astrophysics

Astrophysics

7

Accretion Disks, Binary Stars, Stellar Oscillations, Thomson Scattering, X Ray Stars, Absorption Spectra, Stellar Mass, Stellar Structure, X Ray Binaries

Scientific paper

The internal structure, variable depth, and duration of the dips observed in the low mass X-ray binary 4U1755-33 are suggested to be the result of the partial occultation of an extended source by the oscillating bulge of the accretion disk. The disk oscillations in question may be present in other low mass X-ray binaries containing disks with thick rims or bulges; their observability would depend on the inclination of the system.

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