The slow nova V1819 Cygni (Nova Cygni 1986)

Spectrophotometric and spectropolarimetric observations of the slow nova Cygni 1986 were obtained with the 36-in Pine Bluff Observatory telescope beginning about one week after maximum and continuing for one-two years after maximum. An E(B-V) value of about 0.35 is found. In the months following max...

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Veröffentlicht in:	The Astronomical journal 1989-07, Vol.98, p.297-310
Hauptverfasser:	Whitney, Barbara A., Clayton, Geoffrey C.
Format:	Artikel
Sprache:	eng
Schlagworte:	640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources ABSORPTION Astrophysics BALMER LINES CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS DENSITY ERUPTIVE VARIABLE STARS MORPHOLOGY NOVAE PHYSICAL PROPERTIES POLARIMETRY RADIATION TRANSPORT SPECTROPHOTOMETRY STARS VARIABLE STARS VARIATIONS
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