Positron annihilation spectroscopy of clumpy structures 1. Type II young Supernova remnants
The clumpy structure of the SN 1987A ejecta revealed by numerous IR observations has been described. The simulation of the clump formation in the progenitor star’s explosion was performed. The Sedov self-similar solutions of the problem of a strong explosion were used to construct the model spectra...
| Main Authors: | , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Al-Farabi Kazakh National University
2018-08-01
|
| Series: | Physical Sciences and Technology |
| Online Access: | http://phst/index.php/journal/article/view/147 |