The Astrophysical Journal · 1973 · 81 citations · 0 references
Natural SciencesAstronomyPhysicsAstrophysicsStellar AstronomyUltraviolet AstronomySolar FlaresSolar PhysicsSolar Ultraviolet AstronomyStellar PhotometryUltraviolet SpectroscopyUltraviolet Stellar AstronomyFlare SpectroscopyFlare StarsShock Wave PropagationStellar FlaresTime ResolutionTime-resolved Ultraviolet ObservationsUltraviolet Solar FlaresUltraviolet Stellar Photometry
view Abstract Citations (87) References (22) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS High time resolution studies of UV Ceti. Bopp, B. W. ; Moffett, T. J. Abstract Simultaneous high-speed photometry and time-resolved spectroscopic observations of two large flares on UV Ceti are presented. Marked spectroscopic and photometric differences between the two flares are noted, and spectroscopic and photometric changes during the flares are correlated. For the larger flare, spectrophotometry shows the Balmer lines to contribute 16 percent of the flare intensity in the B-bandpass. The larger flare is compared with the theoretical models of Gurzadyan and Kunkel, and significant discrepancies are found. An interpretation in terms of shock-wave propagation is suggested. Subject headings: flare stars - stars, individual Publication: The Astrophysical Journal Pub Date: October 1973 DOI: 10.1086/152412 Bibcode: 1973ApJ...185..239B full text sources ADS | data products SIMBAD (1) Related Materials (1) Erratum: 1974ApJ...191..289B