Why does the intermediate polar V405 Aurigae show a double-peaked spin pulse?

Monthly Notices of the Royal Astronomical Society

Volumn 353, Issue 2, 2004, Pages 447-452

  Evans, P A ^a   Hellier, Coel ^a  

^a KEELE UNIVERSITY   (United Kingdom)

Author keywords

Accretion, accretion discs; Novae, cataclysmic variables; X rays: binaries

Indexed keywords

MAGNETISM;

ACCRETION: ACCRETION DISKS; HARD X RAY; INTERMEDIATE POLARS; MAGNETIC AXIS; NOVAE CATACLYSMIC VARIABLES; SOFT BANDS; SOFT X-RAY; SPIN PULSE; X-RAYS: BINARIES; XMM-NEWTON OBSERVATIONS;

WHITE DWARFS;

EID: 4544356984     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08073.x     Document Type: Article

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