Article in PDF |
"Peremennye Zvezdy", Prilozhenie, vol. 5, N 6 (2005) |
ISSN 2221–0474 |
Received: 11.11.2005; accepted: 13.12.2005
(E-mail for contact: khruslov@bk.ru)
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Remarks: |
DI And is currently listed in the GCVS as an IS-type star.
According to ROTSE-I data, it is a probable CWB star.
M-m = 0.3P, MaxII = 11.9, MinII = 12.0. The shape of the descending branch is not quite typical. |
Light Curve |