Evolution of the 1-4 μm spectrum of Nova PW Vulpeculae 1984

Monthly Notices of the Royal Astronomical Society

Volumn 279, Issue 3, 1996, Pages 804-826

  Williams, P M ^a   Longmore, A J ^a   Geballe, T R ^b  

^a UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^b UNIVERSITY OF HAWAII   (United States)

Author keywords

Infrared: stars; Novae, cataclysmic variables; Stars: individual: PW Vul

Indexed keywords

ALUMINUM COMPOUNDS; INFRARED SPECTROSCOPY; IRON COMPOUNDS; SILICON COMPOUNDS; STARS; TEMPERATURE;

HYDROGEN LINES; INFRARED: SPECTROSCOPY; INFRARED: STAR; LINE SPECTRA; LINE STRENGTH; LOWS-TEMPERATURES; NOVAE CATACLYSMIC VARIABLES; SPECTRA'S; STAR: INDIVIDUAL: PW VUL; STARS: INDIVIDUAL: PROXIMA CENTAURI;

FLUORESCENCE;

EID: 0242364568     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/279.3.804     Document Type: Article

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