Multifrequency nature of the 0.75 mHz feature in the X-ray light curves of the nova V4743 Sgr

Monthly Notices of the Royal Astronomical Society

Volumn 405, Issue 4, 2010, Pages 2668-2682

  Dobrotka, A ^a   Ness, J U ^b  

^a SLOVAK UNIVERSITY OF TECHNOLOGY   (Slovakia)

^b EUROPEAN SPACE AGENCY   (Spain)

Author keywords

Novae, cataclysmic variables; Stars: individual: V4743 Sgr; X rays: stars

Indexed keywords

LIGHT CURVES; MULTI FREQUENCY; NOVAE CATACLYSMIC VARIABLES; OPTICAL-; SINGLE-FREQUENCY; STAR: INDIVIDUAL: V4743 SGR; STARS: INDIVIDUAL: PROXIMA CENTAURI; V4743 SGR; X-RAY:STARS; XMM-NEWTON;

WHITE DWARFS;

EID: 77955045769     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16654.x     Document Type: Article

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