Multicolour lightcurves of three W UMa systems have been solved using the Wilson-Devinney computer code, modified in order to run on a medium-size minicomputer. The solution confirms the contact hypothesis for these systems, one of which lAQ Tue) has turned out to be of Binnendijk's A-type (deeper minimum produced by the eclipse of the more massive star), and the other two (AE Phe and 44 i Boo) of W-type. A comparison with previous solutions is made.

Determination of parameters of W UMa Systems. I AE Phe, AQ Tue, 44 i Boo / Maceroni, C.; Milano, L.; Russo, G.; Sollazzo, C.. - In: ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES. - ISSN 0365-0138. - 45:(1981), pp. 187-192.

Determination of parameters of W UMa Systems. I AE Phe, AQ Tue, 44 i Boo

L. Milano
Membro del Collaboration Group
;
G. Russo
Membro del Collaboration Group
;
1981

Abstract

Multicolour lightcurves of three W UMa systems have been solved using the Wilson-Devinney computer code, modified in order to run on a medium-size minicomputer. The solution confirms the contact hypothesis for these systems, one of which lAQ Tue) has turned out to be of Binnendijk's A-type (deeper minimum produced by the eclipse of the more massive star), and the other two (AE Phe and 44 i Boo) of W-type. A comparison with previous solutions is made.
1981
Determination of parameters of W UMa Systems. I AE Phe, AQ Tue, 44 i Boo / Maceroni, C.; Milano, L.; Russo, G.; Sollazzo, C.. - In: ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES. - ISSN 0365-0138. - 45:(1981), pp. 187-192.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11588/892562
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