Further observations of PW Vulpeculae

Details Further observations of PW Vulpeculae Further observations of PW Vulpeculae

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...67..111a&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 67, no. 1, Jan. 1987, p. 111-119.

Astronomy and Astrophysics

Astrophysics

8

Novae, Spectrum Analysis, Stellar Spectrophotometry, Absorption Spectra, Astronomical Catalogs, Balmer Series, Line Shape, Near Infrared Radiation, Oxygen Ions

Scientific paper

The paper describes spectrographic observations of Nova PW Vul made at Haute-Provence Observatory during October and early November 1984 in the blue and near infrared. A list of lines and proposed identifications is given in table I. Identified ions are HI, HeI, CI, CII, NI, NII, QI, QII, CaII, TiII and FeII. The P Cygni-type line profile reveals two absorption components systems with velocities around 730 and 1500 km/s.

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