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- W2026160906 abstract "Spectroscopic observations of Nova Centauri 1986 (V842 Cen) in the optical range are presented. The spectra at maximum show strong Balmer and Fe II emission lines with a complex structure, two P Cyg type absorption systems at approximately − 850 km s−1 and − 500 km s−1, and wings extending to ± 1000 km s−1. Later in the nebular phase, strong and broad (FWZ1 ∼ 4000 km s−1) permitted and forbidden emission lines developed a saddle-shaped profile. The characteristics of the nova resemble those of DQ Her. A distance to the nova d = 0.92 ± 0.02 kpc was estimated." @default.
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- W2026160906 date "1989-11-01" @default.
- W2026160906 modified "2023-10-14" @default.
- W2026160906 title "Spectral evolution of Nova Centauri 1986 (V842 Cen)" @default.
- W2026160906 doi "https://doi.org/10.1093/mnras/241.2.311" @default.
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