UBVRI PHOTOMETRY OF CP PUPPIS - A MAGNETIC NOVA

被引：26

作者：

DIAZ, MP ^{[1
]}

STEINER, JE ^{[1
]}

机构：

[1] CERRO TOLOLO INTERAMER OBSERV,LA SERENA,CHILE

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 1991年 / 103卷 / 667期

关键词：

STARS; NOVAE; PHOTOMETRY;

D O I：

10.1086/132913

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Results of about 16 hours of UBVRI photometry of Nova Puppis 1942 are presented. A modulation of the (B-V) color index with the 88-minute orbital period is found. This modulation is interpreted as a possible evidence for a strongly magnetized white dwarf in the system, and a comparison with other novae that are polars or intermediate polars is made.

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页码：964 / 968

页数：5

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