The 1985 outburst of RS Ophiuchi - Spectroscopic results

Details The 1985 outburst of RS Ophiuchi - Spectroscopic results The 1985 outburst of RS Ophiuchi - Spectroscopic results

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989japa...10..237a&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 10, Sept. 1989, p. 237-255.

Astronomy and Astrophysics

Astrophysics

13

Line Spectra, Novae, Optical Emission Spectroscopy, Stellar Envelopes, Ophiuchi Clouds, Spectrum Analysis, Tables (Data)

Scientific paper

Results are reported from visual spectroscopy of the recurrent nova RS Oph, obtained with a Cassegrain spectrograph on the 102-cm reflector at Vainu Bappu Observatory in February-May 1985 (days 32-108 postoutburst). The data are presented in extensive tables and graphs and characterized in detail. It is estimated that the electron density in the ejected envelope decreased from 3 x 10 to the 9th/cu cm on day 32 to 1.8 x 10 to the 8th/cu cm on day 108; the temperature in the coronal line region decreased from 1.5 to 1.1 million K over the same period.

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