Evidence for ablated flows in the shell of the nova DQ Herculis

Monthly Notices of the Royal Astronomical Society

Volumn 380, Issue 1, 2007, Pages 175-180

  Vaytet, N M H ^a   O'Brien, T J ^a   Rushton, A P ^a  

^a UNIVERSITY OF MANCHESTER   (United Kingdom)

Author keywords

Novae, cataclysmic variables; Stars: individual: DQ Herculis; Stars: winds, outflows

Indexed keywords

STARS;

EQUATORIAL EXPANSION; EXPANSION VELOCITY; HIGH RESOLUTION; NARROW BANDS; NOVAE CATACLYSMIC VARIABLES; SPECTRA'S; STAR: INDIVIDUAL: DQ HERCULIS; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: WINDS OUTFLOWS; WILLIAM HERSCHEL TELESCOPES;

SHELLS (STRUCTURES);

EID: 34548074940     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12057.x     Document Type: Article

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