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Sagittarii (Ch. 6 8 I 7) and Nova Aquilae (Ch. 6932), were found in the regular examination of the Draper Memorial photographs, and probably all of them would otherwise have escaped detection. Two, Nova Aurigae (T Aurigae, Ch. 1 9 5 3 ) and Nova Persei No. 2 (Ch. 1 2 2 6 ) , were bright, and were found visually by Dr. Anderson. The first of these 3864 might have escaped detection here, although numerous early charts were obtained which showed that it was visible to ' the naked eye during seven weeks before its discovery. The spectrum of Turner's Nova is so conspicuous on the plate taken on March 2 5 , that when this plate was developed and examined it would doubtless have been found on it here, but for the prompt discovery and announcement by Professor Turner.") 428 De'couverte d'une variable nouvelle 16.1903 Monocerotis. En etudiant les photographies prises par M. S. Blajko, Mme. L. Ceraski a trouvC une variable nouvelle dont la position approchCe est la suivante: 1855.0 a = q h r o m o d = + I O Z Z ' 1900.0 a = 7 " 1 z m 1 3 d = +1018'. Sur une de nos photographies, de fCvrier 1 8 9 9 , elle est 9.3 gr.; sur d'autres, elle est plus faible. J'ai constate MOSCOU, 1903, le 30 mars/ 1 2 avril. Prof. l d ? Cernski. qu'A present l'etoile est invisible, elle est de 1 3 ~ gr. ou encore inferieure.
๐ SIMILAR VOLUMES
Vergleichsterne. a BD. +3001302 (9m2, ang. 9m1) 6 3 +30.1306 (8.6) c D +30.1316 (9.0, ang. 9.1) d s +30.1320 (8.9, ang. 8.6) c ; ) +29.1328 (9.2, ang. 9.3) f P +30.1321 (9.2, ang. 9.5) g +30\*1309 (9.4) April 13. 8h M. Z. Wien. Nova 4 Stufen heller als a, 2 Stufen schwgcher als b, 4 Stufen heller al