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A Spectroscopic Survey of Recurrent Novae at Minimum1

Published online by Cambridge University Press:  12 April 2016

H.W. Duerbeck  and
W.C. Seitter
H.W. Duerbeck
Affiliation:
Astronomisches Institut der WestfälischenWilhelms-Universität, Münster, F.R.Germany
W.C. Seitter
Affiliation:
Astronomisches Institut der WestfälischenWilhelms-Universität, Münster, F.R.Germany

Extract

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From 1986 to 1988 optical spectroscopy near minimum of all then established recurrent novae (excluding recurrent X-ray novae such as V616 Mon and V404 Cyg) was carried out with the 3.6 m and 1.5 m telescopes of ESO, using EFOSC with CCD and the Cassegrain spectrograph with CCD or IDS, respectively. Flux-calibrated spectra of the six objects are shown in Figs, 1a – f. The most recent recurrent nova, V745 Sco, is included in the present discussion, because 1 month after outburst it had already reached a very late stage of outburst evolution. A spectrum of V745 Sco is shown in Schwarz et al. (1989).

Type
4. Related Objects
Information
International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 425 - 426
Copyright
Copyright © Springer-Verlag 1990

Footnotes

1

Based on observations collected at the European Southern Observatory, La Silla, Chile

References

Kenyon, S.J., 1986. The Symbiotic Stars. Cambridge: Cambridge University Press.Google Scholar
Schmid, H.M., 1989. These proceedings.Google Scholar
Schwarz, H.E., Duerbeck, H.W., Seitter, W.C., 1989. These proceedings.Google Scholar
Sekiguchi, K., Catchpole, R.M., Fairall, A.P., Feast, M.W., Kilkenny, D., Laney, C.D., Lloyd Evans, T., Marang, F., Parker, Q.A., 1989. Mon. Not. R. astr. Soc. (in press).Google Scholar
Sekiguchi, K., Feast, M.W., Whitelock, P.A., Overbeek, M.D., Wargau, W., 1988. Mon. Not. R. astr. Soc., 234, 281.CrossRefGoogle Scholar