Optical spectroscopy of nova LMC 1988 No. 2 during its early decline stage

Details Optical spectroscopy of nova LMC 1988 No. 2 during its early decline stage Optical spectroscopy of nova LMC 1988 No. 2 during its early decline stage

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.241..827s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 241, Dec. 15, 1989, p. 827-837.

Astronomy and Astrophysics

Astronomy

7

Magellanic Clouds, Novae, Stellar Spectra, Visible Spectrum, Astronomical Spectroscopy, Light Curve, Line Spectra, Radial Velocity

Scientific paper

This paper presents the results obtained from optical spectroscopy of nova LMC 1988 No. 2 made at the SAAO. It was a very fast nova (t2 = 5 d) of large amplitude (greater than 11.2 mag), and the visual maximum reached m(v) = 10.3 on October 13.75, 1988 (UT). A spectrogram taken 1.34 d after the maximum showed strong Balmer, He I, and Fe II lines with P Cyg profiles.

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