By Hilmar W. Duerbeck
4. Census of includes info on 277 items. 137 (50%) of them are stars whose outburst spectra or unambiguous minimal features classify them as novae past doubt. 123 of them may be pointed out at minimal. seventy eight (28 percent) are stars with amplitudes and lightweight curve types which makes nova classifi cation most probably. 60 of them may be pointed out at minimal. therefore, seventy eight % ofthe items during this catalogue are proven and suspected classical novae. sixteen (6%) have homes suitable with either novae and comparable gadgets. 15 are pointed out at minimal. additionally, and atlas comprises facts on 12 (4 percent) dwarf novae of lengthy cycle size or suspected dwarf novae for which just one outburst has been saw. Examples are WZ Sge and CI Gern. 6 (2%) recurrent novae or suspected recurrent novae are indexed. Examples are T CrB and AS Psc. 6 (2%) X-ray novae are indexed. Examples are V616 Mon and KY TrA. 6 (2%) symbiotic stars and symbiotic novae are indexed. Examples are RT Ser and V352 Aql. eleven (4 percent) Mira stars or suspected Mira stars, which at a while have been believed to be novae, are indexed. Examples are V607 Aql and V927 Sgr.
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Extra info for A Reference Catalogue and Atlas of Galactic Novae
Guarneri, C. Bartolini, F. Giovanelli, AA 34 (1984) 473. Identification: from Harvard plate MC 40022, taken 1978 September 10. Classification: fast nova, well observed from the ultraviolet to the infrared. 4271 d were observed (H. Ritter 1984). M V1760 eyg (N Cyg 1980, Honda's variable) Discovered by M. Honda, Japan, 1980 November 29, as a 10m star (lAU Cire 3546). ) LCT:M from published precise positions. Mira variable with P = 298 d (E. Waagen, lAU Cire 3553 (l980)) THE CATALOGUE 55 NB N Cyg 1986 Discovered by M.
Very slow nova with well-documented light curve. 36 HILMAR W. DUERBECK N N Car 1953 (NSV 04884) Discovered br L. Perek as emission-line object on objective prism plates of the Tonantzintla Schmidt telescope, taken 1953 February 8/9 and 1953 March 10/11 (BAC 11 (1960) 256). 726 (ESO) (L. ) LCT: ? Classification: H. W. Duerbeck, IBVS 2502 (1984). L. Perek, BAC 11 (1960) 256 - descr. from Harvard plates B 76601, taken 1953 January 23/24, and B 76679, taken 1953 March 19/20. nova, poorly known. N Car 1971 N Light curve: Spectroscopy: Identification: Discovered by D.
Hjellming, C. M. Wade, N. R. Vandenberg, R. T. Newell, AJ84 (1979) 1619. B. Zellner, M. D. Morrison, AJ 76 (1971) 645; J. Arsenievic, A. Polarization: Kubicela, IBVS 495 (1970); E. T. Belonkon', O. S. Shulov, AG LGU Trudy 30 (Ser. Mat. Nauk 50, 1974) 103. Nebular Shell: D. Soderblom, PASP 88 (1976) 517; L. Kohoutek, MN 196 (1981) 87p; J. Solf, ApJ 273 (1983) 647. 2141674 (A. Bruch, PASP 94 (1982) 912) supersedes all previous determinations (H. Ritter (1984». UVobservations: J. Krautter, G. Klare, B.