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 'mmiam f<r.iTfatftuiimmm ttrntjum m.msiiiv^nmasiss^met 
 

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 2 
 
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 wmmmmmmm 
 
 SS! 
 
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 MICROCOPY RESOIUKON TEST CHART 
 
 AMil u'd ISO TEST CMABI N„ ] 
 
 1.0 
 
 .25 
 
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 32 
 
 1.4 
 
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 ^ APPLIED IIVMGE Inc 
 
PUBLIC' 
 
 (iV 
 
 Bominion !lsitrop{)] 
 
 \'i( re 
 Vol. [, : 
 
 THE ORBITS OF THi: Sl'KC 
 
 OF HOS 
 
 HY W. K. 
 
 This star (I'JOO a = 19'' 30 ■4'", 5 = +r>A 
 was found to be u binarj' from the double Vnu 
 nine plates were secured during the suninier, 
 present solution. These four, taken befoiv t 
 a phase in the orbit where the siiectru are partiii 
 Of the remainhig twenty-five all but f(jur h 
 the determination of the orbit rests on the wji 
 oji Seed 30 enmlsion with the sinf^le jirisin s] 
 central ray X42()0 of 25-7 ajigstronis per niillii 
 
 The spectra of the two conij)onents are 
 being barely sufficient to eiuible one to toll 
 set of lines belongs. The lines of both comp 
 dozen on the average were measured in each 
 the probable error of a plate for component 1 
 ±2 1, and for the other ±2-5 km. per sec. 
 nearly e<iual, component 2 having a ma.ss Ui) 
 
 7C284- 1 
 
'M:Jt^ 
 
 'lINivfRMu '*.-^'i'^* 
 
 ., ,r,HV'C 
 
 P 
 
 \r 
 
 - 1 V 198^ 
 
 B!B -K)TH^-OUyJ^ 
 
 UJCATIOXS 
 
 i>r iHi. 
 
 ropfjpgiral (^(jserbatorp 
 
 ■ICIORIA 
 
 'ol. I, \<1. 1» 
 
 Sl'KCTKOSCOl'lC COMl'OXKNTS 
 
 ■ lioss r>02v, 
 
 \\. K. IIAUl'EU 
 
 = +.j4M4', photographic magnitude G -3, type P'ij) 
 hie lines shown on the first plate made. Twenty- 
 imner, all but four of which have been used in the 
 )efore the ai)pr<iximate ])erioil was known, fall at 
 ' partially sui)erposed and he... _ are unmeasurable. 
 four have both components measurable, so that 
 the wjuivalent of forty-ix plates. All were made 
 irism sjjectrograiih, wliich has a dispersion at the 
 T niillinietrc. 
 
 Its are <|uite similar, the difference in intensities 
 () tell from insjjcction to which component each 
 
 I comi)oj»'nts arc fuzzy in nature, but as about a 
 
 II each case, a fairly reliable result was obtained, 
 ncnt 1 (the one with the more intense lines) being 
 r see. The masses, as may be expected, are very 
 iiss 0-'.»8tJ times that of component 1. 
 
1A8 
 
 PUBLICATIONS OF THE DOMINION ASTROPHYSICAL OBSERVATORY 
 
 In the tublo of ohsorvations following the i)hases arc reckoned from the final value 
 if iHTJastron pas>aKc u>iiin the corrected period 7 ti:{s:5 days. 
 
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 -117 4 
 + 44 3 
 + 390 
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 + 121 
 + 30 
 
 -107-7 
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 - 57 5 
 -110-7 
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 + 42-5 
 
 - 95 2 
 -120 3 
 
 I 
 
 9 
 5 
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 14 
 10 
 8 
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 9 
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 The period wa.s obtained early in the observations, thus avoiding to a large extent 
 useless plates at phases where the lines would be hopelessly mixed. In addition, this 
 knowledge of the general form of the curve made po.ssible the securing of separated spectra 
 close to the crossing points by narrowing the collimator slit from its usual width of 
 ().")1 mm. Nicely resolved lines were secured where the difference in velocity was of 
 the order of 70 km. per sec, and in one case a difTerence of tjO km. gave lines clearly double 
 in the violet region. 
 
 Krom the jireliminary elements gi\en later observation etjuations were built up ac- 
 cording to the notation of l.ehmann-Filhes, modihed to suit cases of double spectra*, 
 and a least — .s()uares solution effected. .\s no early observations existed whereby the 
 preliminary value of the period might be corrected, this term was also included in the 
 sdhition. This i)ractically necessitated treating all the observations separately, and only 
 wht re they were taken on one night or where they fell on a smooth part of the curve 
 was this principle dei)arted from. In this connection the four plates showing single lines 
 
 ' Ddruiiiioii t Kisi I viitiin I'liljlii-atioiis, Vol. I, paKi- 327. 
 
<l»SKH\ AlluNS OK HOS.X .ifCti 
 
 IM 
 
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 into onr iwirriml pliK'c. Hy iiiakiiiK ihr following traiisforiiiatiims a srt of Ha (if)s('r\'ati()ii 
 p(Hiations involvin); the 7 iiiiiviiowns 7, Ki, K., r, ui. V and T wrrc t)uilt iq). TJir weights 
 of each arc as given in the last column. 
 
 X = «7 
 y = «K, 
 7. = SK, 
 n = ".I2 «« 
 
 V = ifj «U) 
 
 « = |;M':ii()4l f> I' 
 1 = |2ii:w-)| «T 
 
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 1 
 
 .1. tin 1 
 
 •M rjkm • (1 71 km 
 
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 1 
 
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 1 H.M O 
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 Domi 
 
 inion .\.sfrophvsiral Obsprvaforv, 
 Vicffiria, B ('. 
 Nov. 7, 1!M!». 
 
 
tej ^.:.'»^ei>-i - -^rar.. 
 
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