
TY  - JOUR
A1  - Allakhverdiyev, AO 
A1  - Guseinov, OH 
A1  - Yusifov, IM 
T1  - Spatial Distribution of Pulsars and Supernova Remnants
JF  - Australian Journal of Physics
JO  - Aust. J.  Phys.
Y1  - 1987
VL  - 40
IS  - 6
SP  - 837
EP  - 846
KW  - 
UR  - https://doi.org/10.1071/PH870837 
N2  - We show that the burst of Type I supernovas occurs about 108 years after the birth of the progenitor. This duration results in the main by the delay of the burst after the formation of a white dwarf of about one solar mass in a close binary system. The mass of the main component of this system is about 8M0 , and the mass of the secondary about 3M0 . These stars complete their evolution as Type I supernovas and are distributed along the galactic plane. Pulsars are formed about 107 years after the birth of their progenitors, and are accompanied by a Type II supernova. Pulsars therefore have an annular distribution in the Galaxy. 
ER  -

