In the follovving a method is proposed to determine the mean coefficient of interstellar absorption and the mean extinction from the observed spectroscopic parallazes, the radial velocity and the proper moti- ons. The distribution $ (x, y, z/S) is assumed to be constant in the immedi- ate surroundings of the sun. This is a reasonable assumption. Therefore the velocity Iaw must be a constant along any axis. independent of its orienta- tion. In different areas of the sky it is cor.venient to adopt as axis the radi- us vector and the direetion perpendieular to and tangent to the cireles »and S The equations of motion containing a are derived. From these the nume- rical values of a can easily be derived.
Birincil Dil | İngilizce |
---|---|
Konular | Matematik |
Bölüm | Research Article |
Yazarlar | |
Yayımlanma Tarihi | 1 Ocak 1959 |
Gönderilme Tarihi | 1 Ocak 1959 |
Yayımlandığı Sayı | Yıl 1959 Cilt: 10 |
Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics.
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