The enigma of the oldest 'nova': The central star and nebula of CK Vul

Monthly Notices of the Royal Astronomical Society

Volumn 378, Issue 4, 2007, Pages 1298-1308

  Hajduk, M ^a   Zijlstra, Albert A ^b   Van Hoof, P A M ^c   Lopez, J A ^d   Drew, J E ^e   Evans, A ^f   Eyres, S P S ^g   Gesicki, K ^a   Greimel, R ^h   Kerber, F ⁱ   Kimeswenger, S ^j   Richer, M G ^d  

^a NICOLAUS COPERNICUS UNIVERSITY   (Poland)

^b UNIVERSITY OF MANCHESTER   (United Kingdom)

^c ROYAL OBSERVATORY OF BELGIUM   (Belgium)

^d UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^e IMPERIAL COLLEGE LONDON   (United Kingdom)

^f KEELE UNIVERSITY   (United Kingdom)

^g UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

^h ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

ⁱ EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^j UNIVERSITY OF INNSBRUCK   (Austria)

more..

Author keywords

Binaries: general; Planetary nebulae: general; Stars: AGB and post AGB; Stars: evolution; Stars: individual: CK Vul; Stars: mass loss

Indexed keywords

IONIZATION OF GASES; RADIO ASTRONOMY; SUPERNOVAE;

BINARIES:GENERAL; CLASSIFIEDS; PLANETARY NEBULAE:GENERAL; RADIO IMAGES; STAR: EVOLUTION; STAR: INDIVIDUAL: CK VUL; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MASS-LOSS; STARS:AGB AND POST AGB; THERMAL PULSE;

WHITE DWARFS;

EID: 34547352134     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11825.x     Document Type: Article

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