Eight-color photometry of Nova Vulpeculae 1984b

Details Eight-color photometry of Nova Vulpeculae 1984b Eight-color photometry of Nova Vulpeculae 1984b

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..832b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Nov. 1985, p. 832-837) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Nov.-Dec

Astronomy and Astrophysics

Astronomy

5

Infrared Photometry, Novae, Spectral Energy Distribution, Stellar Spectrophotometry, Ubv Spectra, Constellations, Light Curve, Stellar Cores, Stellar Envelopes, Stellar Evolution

Scientific paper

The spectral energy distribution of Nova Vul 1984 No. 2 about 15 d after
maximum light is derived from photoelectric UBVRIJHK photometry using a
triple-crosswire technique. The stellar core had a B2 Ia spectrum, while
the detached envelope was F5-F8 I. Up to wavelength 2.5 microns there is
no evidence of a dust shell.

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