The radius of the accretion disc in Z Cha between outbursts

Details The radius of the accretion disc in Z Cha between outbursts The radius of the accretion disc in Z Cha between outbursts

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.220p..23o&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 220, May 15, 1986, p. 23P-26P. Research supported by th

Astronomy and Astrophysics

Astronomy

58

Accretion Disks, Dwarf Novae, Stellar Mass Accretion, Stellar Structure, Eclipsing Binary Stars, Radii

Scientific paper

Published measurements of the radius of the accretion disc in the dwarf
nova Z Cha and new observations made at significant times during the
outburst cycle, exhibit a decline in disc radius between outbursts,
similar to that found for U Gem. The relationship has least scatter when
considered as a function of fractional time between outbursts.

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