Extending emission-line Doppler tomography: Mapping modulated line flux

Monthly Notices of the Royal Astronomical Society

Volumn 344, Issue 2, 2003, Pages 448-454

  Steeghs, D ^a,b  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

Author keywords

Accretion, accretion discs; Binaries: Close; Line: Profiles; Novae, cataclysmic variables; Stars: Individual: IP Peg; Techniques: Spectroscopic

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; MAPPING; MODULATION; SIGNAL TO NOISE RATIO; STARS; TOMOGRAPHY;

ACCRETION FLOW; ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; DOPPLER TOMOGRAPHY; EMISSION LINES; EMISSION SOURCES; LINE: PROFILES; NOVAE CATACLYSMIC VARIABLES; STARS:INDIVIDUAL:IP PEG; TECHNIQUES: SPECTROSCOPIC;

REPAIR;

EID: 0141921434     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06917.x     Document Type: Article

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