By Hilmar W. Duerbeck
4. Census of includes info on 277 gadgets. 137 (50%) of them are stars whose outburst spectra or unambiguous minimal features classify them as novae past doubt. 123 of them might be pointed out at minimal. seventy eight (28 percent) are stars with amplitudes and lightweight curve types which makes nova classifi cation most likely. 60 of them can be pointed out at minimal. hence, seventy eight % ofthe items during this catalogue are proven and suspected classical novae. sixteen (6%) have homes appropriate with either novae and similar items. 15 are pointed out at minimal. in addition, and atlas includes 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 it slow have been believed to be novae, are indexed. Examples are V607 Aql and V927 Sgr.
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Extra resources for A Reference Catalogue and Atlas of Galactic Novae
090 (POSS, at limit) (M. and G. ) LCT: ? M. and G. Wolf, AN 169 (1905) 415; K. Himpel, E. Jansch, HZ 25 (1943) 105. M. and G. Wolf, AN 169 (1905) 415; K. Himpel and E. '7) on 1943 September 2 (HZ 25 (1943) 105). 2m telescope on 1984 August 21/22, were used. The original position given by Wolf and Wolf seems to be erroneous. The observation of 1943 September 2 is doubtful. The large amplitude makes nova c1assification likely, however, no spectroscopic information is available. Intergalactic object?
Stratton, ASPO Camb 4 (1936) 133 - phot, ident, rv; D. B. Spectroscopy: McLaughlin, Miehigan Publ6 (1937) 107 - phot, ident, rv; F. J. M . Stratton, W. H. Manning, Atlas of Spectra of Nova HercuIis, Cambridge (1939) - phot; C. Bertaud (1945) - rv; C. Sneden,D. L. Lambert, MN 170 (1975) 533-CNisotopes; E. R. Mustel, L. 1. Baranova, AZh 42 (1965) 42 = Sov Astr 9 (1965) 31 abundances, L. 1. Antipova, AZh 46 (1969) 366, AZh 48 (1971) 288 = Sov Astr 13 (1969) 288, Sov. Astr 15 (1971) 225 - CN bands, H lines; R.
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.