Chandrasekhar, C. ; Münch, G. (1951) The theory of the fluctuations in brightness of the Milky Way. III Astrophysical Journal, 114 . pp. 110-122. ISSN 0004-637X
![[img]](https://repository.ias.ac.in/style/images/fileicons/application_pdf.png)
|
PDF
- Publisher Version
343kB |
Official URL: http://adsabs.harvard.edu/abs/1951ApJ...114..110C
Related URL: http://dx.doi.org/10.1086/145455
Abstract
In this paper the integral equation (derived in Paper I) governing the fluctuations in brightness of the Milky Way is explicitly solved for the case in which the system extends to a finite distance in the direction of the line of sight and when all the clouds are equally transparent, The derived theoretical distributions are illustrated.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to American Astronomical Society. |
| ID Code: | 74387 |
| Deposited On: | 12 Dec 2011 05:07 |
| Last Modified: | 18 May 2016 18:49 |
Repository Staff Only: item control page
