共 50 条
- [31] Observations of the comet Brooks (a 1904) made at the observatory of Alger, at the equatorial bent at an angle of Om, 318. COMPTES RENDUS HEBDOMADAIRES DES SEANCES DE L ACADEMIE DES SCIENCES, 1904, 138 : 1147 - 1147
- [32] Observations of the Borrelly-Brooks comet, made at the Brunner equatorial of the Lyon observatory COMPTES RENDUS HEBDOMADAIRES DES SEANCES DE L ACADEMIE DES SCIENCES, 1900, 131 : 373 - 374
- [33] Astronomy - Observations made of the Schjellerup comet (1922a), made with the curved equatorial of the Nice Observatory. COMPTES RENDUS HEBDOMADAIRES DES SEANCES DE L ACADEMIE DES SCIENCES, 1922, 174 : 1333 - 1333
- [34] Observations of the Borrelly comet, made at the observatory of Algers, with the equatorial bent to 0m, 318 of opening COMPTES RENDUS HEBDOMADAIRES DES SEANCES DE L ACADEMIE DES SCIENCES, 1900, 131 : 406 - 406
- [35] Observations of the Kiess comet (1911b), made at the grand equatorial of the Bordeaux Observatory. COMPTES RENDUS HEBDOMADAIRES DES SEANCES DE L ACADEMIE DES SCIENCES, 1911, 153 : 165 - 166
- [36] Observations of the comet Zlatinsky (1914b) made at the bended equatorial of the Nice Observatory. COMPTES RENDUS HEBDOMADAIRES DES SEANCES DE L ACADEMIE DES SCIENCES, 1914, 158 : 1480 - 1481
- [37] Observations of the Kiess comet (1911b) made at the Brunner equatorial of the Lyons Observatory. COMPTES RENDUS HEBDOMADAIRES DES SEANCES DE L ACADEMIE DES SCIENCES, 1911, 153 : 378 - 378
- [38] Observations of the Quenisset comet and the Brooks comet at the big equatorial (0(m),38) of the Bordeaux Observatory. COMPTES RENDUS HEBDOMADAIRES DES SEANCES DE L ACADEMIE DES SCIENCES, 1911, 153 : 619 - 621
- [39] Astronomy - Observations of the Skellerup comet (1922a), made with the curved equatorial of the Besancon Observatory. COMPTES RENDUS HEBDOMADAIRES DES SEANCES DE L ACADEMIE DES SCIENCES, 1922, 174 : 1332 - 1333
- [40] Observations of the Giacobini comet (1905c) made at the Brunner equatorial (0(m),16) of the Lyons Observatory. COMPTES RENDUS HEBDOMADAIRES DES SEANCES DE L ACADEMIE DES SCIENCES, 1906, 142 : 31 - 31