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Volumn 417, Issue 3, 2004, Pages 1063-1074

Spiral shock detection on eclipse maps: Simulations and observations

Author keywords

Accretion, accretion disks; Line: formation; Methods: data analysis; Shock waves; Stars: individual: IP Pegasi; Stars: novae, cataclysmic variables; Techniques: photometric

Indexed keywords

COMPUTER SIMULATION; DATA REDUCTION; DOPPLER EFFECT; MAPPING; PHOTOMETRY; SHOCK WAVES; SIGNAL TO NOISE RATIO; TOMOGRAPHY;

EID: 4544228078     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20035643     Document Type: Article
Times cited : (7)

References (27)
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    • Hameury, J.-M. 2002, in Physics of Cataclysmic Variables and Related Objects, ed. B. T. Gaensicke, K. Beuermann, & K. Reinsch (San Fransisco: Astronomical Society of the Pacific), ASP Conf. Ser., 261, 377
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  • 12
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    • Steeghs, D. 2001, in Astrotomography: Indirect Imaging Methods in Observational Astrophysics, ed. H. Boffin, D. Steeghs, & J. Cuypers (Heidelberg: Springer-Verlag), Lecture Notes in Phys. Ser., 573, 45
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    • Cataclysmic Variable stars
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.