On the decline stage of Nova V 3888 SGR /1974/

Details On the decline stage of Nova V 3888 SGR /1974/ On the decline stage of Nova V 3888 SGR /1974/

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....61..601v&link_type=abstract

Astronomy and Astrophysics, vol. 61, no. 4, Nov. 1977, p. 601-603.

Astronomy and Astrophysics

Astrophysics

1

Novae, Stellar Spectrophotometry, Ubv Spectra, Color, Light Curve, Stellar Luminosity

Scientific paper

Photoelectric UBV and uvby photometry of V 3888 SgrNova Sgr 1974 was obtained covering 25 days of its decline stage. The light curve and the color variations are described and compared with the spectrum. V 3888 Sgr seems to be a fast nova with a slightly abnormal light curve showing a rapid early decline but an extended transition state. Its maximum brightness is estimated to be about 7.5 m, its amplitude not less than about 13.5 and its distance 3.5 kpc.

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