Nova vulpeculae 1984 N 2 in 1985

Data from UBVRIJHK photometric, UBVRI polarimetric, and spectrophotometric observations of QU Vul obtained between May and December 1985 are reported. A dust shell model is discussed which can explain the observed properties of the nova. Results for M sub v, effective temperature, and radius are giv...

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Veröffentlicht in:	Astrophysics and space science 1988-11, Vol.149 (1), p.63-71
Hauptverfasser:	BERGNER, YU. K, MIROSHNICHENKO, A. S, YUDIN, R. V, YUTANOV, N. YU, DZAKUSHEVA, K. G, ILYIN, V. V, KURATOV, K. S, MUKANOV, D. B
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology Novae, dwarf novae, recurrent novae, and other cataclysmic (eruptive) variables Stars Variable and peculiar stars (including novae)
Online-Zugang:	Volltext
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Beschreibung
Zusammenfassung:	Data from UBVRIJHK photometric, UBVRI polarimetric, and spectrophotometric observations of QU Vul obtained between May and December 1985 are reported. A dust shell model is discussed which can explain the observed properties of the nova. Results for M sub v, effective temperature, and radius are given for several times. (R.R.)
ISSN:	0004-640X 1572-946X
DOI:	10.1007/BF00640466