## 334 can generally be made quite small with the expenditure of but little time. It remains then to set the instrument so that the azimuth error shall not exceed say five or six degrees. For symmetry observe four stars not far from the zenith reversing between the pecond and third. These stars sh
Beobachtungen des Cometen II 1873 Angestellt auf der Sternwarte Arcetri bei Florenz.
β Scribed by Wilh. Tempel
- Publisher
- John Wiley and Sons
- Year
- 1878
- Tongue
- English
- Weight
- 159 KB
- Volume
- 93
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
β¦ Synopsis
Der Stern in B.D. 19"45"5587
Heia's Uranometrie als 5ter Gr6sse verzeichnet, und im Die scheinbaren Oerter der Vergleichsterne wurden folgendermaassen angenommen, wobei ich bemerke, dass der unbekannte Stern d von mir genghert nach 2 Nachbarsternen bestimmt ward. d = 16h12m18865 -1 7 O 4 0 17"2 fehlt bei Argelander e =
π SIMILAR VOLUMES
a ' Schjellerup 954 j-46 ( : z z 346'39'40"17 d r-+ 10~18'31"S red. + 64"72 c Lamont 3330 346 26 0 0 . 2 0
lyith thc aid of the approximate elements published in Circular m n Herliner Jahrbuch Nr. I 2 I tlic foliowing normals were obtained from all the observatioiis made during the first opposition.
446 7.0 3.3 5.4 4.0 4.4 5.0 4.4 4.4 The length of a period at the time of Hevel's observation was 35 8.6 days upon the hypothesis A and 380 days upon hypo-