ASTRONOMY. 213 



Stars (Motion of) in the lino of ,sij;lit— Coutimicil. 



Vogicl(H. C.) lic-stiiiuuiujg dor IJewegiinj;- von Storncn mi Visionsradins. As- 

 tion. Naclir., lll>: '.>/. 



Bestinmumg dcr Bewegnng von Stci-ueu im Visionsradiu.s dnreli spectro- 



giapbische Beobac'htnng. Mem. Soc. spettrscp. itai., 17: i!".?. 



Sun. Sec, uIho. Conosx; PuoMixr.xcKs ; Spectkum; Sun (Diamctca- of), etc. 



r'i,.vMMAKi()X(C.) Lcsgrandt's manifestations do I'activito sola! re. il. L'Astron., 

 7: 1-21-133. 



Line annde de Thistoire dn soleil. il. L'Astron., 7: 201-213. 



FuiTZ (H.) Beitriige znr Bezieliung irdisclier Erscheinnngen znr SoniKMitbiitig- 



kcit. Sirins, 21 : 20G-210, 217-222, 245-240. 

 Sciiur.z (J. F. H.) Znr Sonnenphysik. 11. 1 pi. Astron. Naclir., 119: 225-242. 

 Si:arlk(A. ) jVtniosplioric economy of solar radiation. Proc. Am. Acad. Arts and 



Sc, 2(5-20. Also, Reprint. 



Sun (Diameter of). 



Wkllmax (V.) Eiullnss der Blendgliiser bei Beobaehtnngen des Sonnendnrch- 

 messers. Astron. Naclir., 119: 241. 



Sun (Rotation of). 



Cuuw (H. ) Period of the rotation of the snn as determined by the spectroscope. 



Am. J. Sc, 135: 151-159. 

 WiLsiXG (J.) Ableitung der Rotationsbevvegnng der Sonne ans Positionsbestim- 



muugeu vou Fackelu. Astron. Naehr., 119 : 311-31G. 

 Sun (Statistics of facnhe, prominences, and spots). 



1''lammarion (C.) Flnct nations do I'activite solairo depnis le (hirniqr maximum 



de 1H"*3-'81 Jusqu'an dela dn dernier niinimnm. Taelies facnlcs, I'irnptions et 



magnet isine terrestre. il. L'Astron., 7: 41-53. 

 SiH)Kiii:u (A.) Verschiedenheit der Hiinligkeit d<3r Sonnentleckon auf der nord- 



lichen nud siidlichen Ilalbkngel in den Jahren IsSiJund 1^37. Astron. Nachr., 



118: 307. 

 Tkten's(0.) Sonnenllecke im Jahre isd" nacli den Beobachtnngen zn O'Gyalla. 



Astron. Nachr., 119: 207. 

 WoLii' (R.) Sonnen-Statistik des .lahres 1887. Astron. Nachr., 118: 307. 



Sun-spots. 



Bossi (B.) Le macchie solari ; canse ed etietti. Sni terremoti avvennti e fnturi 

 comedaiiredizionideir autore. 3. ed.,eii]. lUip. lliino. (lienova, 1888 .(M. 1.50) 

 Fayk (H.) Remarquessur nne objection de M. KhandrikolV:\ l.i thdoriodestacbeH 

 et des iirotnbdiances solaires. Conii»t. Rend., lOC): 399-103. 



Taches et protub<!rances solaires. L'Astron., 7 : 89-93. 



Tables (Loga.rithmic). 



Nkll(A. M.) FiinfstelligeLogarithmen . . . (>. cd. 19+104 p. Hvo. Darmstadt, 



1S88 '. (M. 1.80) 



Taschkent Observatory. 



PoMKKAXiZEFF (H.) I.,atitnde de Tobservatoire de TacihktMit. Astron. Nachr., 

 119: 317. 



[MEVIonis of tlic Tasclikfiit Jistioiioiiiic.il and jiliysical <)l>ai'rvat(»ry. Piiljlicatioii II.] 104 

 p. 4to. MocKiiii, 1888. 



Telegrams (Astronomical). Sec Code (Astronomical). 

 Telescopes. /See, a?8o, Equatoisiai.s; Mirrors; Oiuectives. 



Ckossley (E.) Improved centering tnite for refhicting telescopes. Month. Not., 



48: 280. 

 GKUBi5(n.) Good astronomical telescopes. Sid. Mess., 7 : 10(5,259. 

 Harkxess (W.) Visibility of objects as conditiontid by their magnitnde and 

 brightness with a))plications to the theory of telescopes. Abulr. : I'roc. Am, 

 Assn. Adv. Sc, 3G: G4. 



