Course in Astrophsics And Stellar Astronomy volume 11

Cover Course in Astrophsics And Stellar Astronomy volume 11
Course in Astrophsics And Stellar Astronomy volume 11
B P Gerasimovich
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-^JZL _ ___. \Q I G"m 3 The universal and accurate methods of -Teasurement and reduction of astro- grams expounded ai ove sometimes require a great expenditure of time* But there are oases when it is necessary to determine as quiekly as possible the position of a single celestial object (comet, planet, variable star, et) even If the accuracy ias to suffer somewhat* In such eases it is often sufficient to Inter p >1 te the sought position of the object between two (or three) basic stars* The mea...surements are also simplified, they do not require a previous orientation of t' e plate, Suoh interpolation methods are those of Kaiser, Reger, Wolf, Schlo singer* Let K be an object on t':e rlute the position of which needs to be de- termined (Fig* 14)* Let us select two basic stars! (l)and(2) such that object K be, as close as possible to the line (l) - (2), Let us pass through star (2) the celestial meridian and through star (1) the parallel of declination (we shall neglect the error of projection of the sphere on a plrme)* He measure tho dif- ference of the coordinates with respect to some axes X, Y: Ax and Ay for the pair of basic stars.

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