On the galactic distributions of radio pulsars and plasma density | Zendy

A. Ankay | Zendy; E. Yazgan | Zendy; Pinar Kütükcü | Zendy

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On the galactic distributions of radio pulsars and plasma density

Author(s) -

A. Ankay,

E. Yazgan,

Pinar Kütükcü

Publication year - 2016

Publication title -

serbian astronomical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.196

H-Index - 16

eISSN - 1820-9289

pISSN - 1450-698X

DOI - 10.2298/saj1693001a

Subject(s) - physics , pulsar , astrophysics , source counts , dispersion (optics) , measure (data warehouse) , latitude , plasma , longitude , astronomy , galaxy , optics , redshift , database , quantum mechanics , computer science

A brief review of distance measurement methods for some astronomical sources is presented. Galactic plasma density distribution as related to the distribution of radio pulsars is discussed and a method for constructing relations between dispersion measure and distance for Galactic radio pulsars in small solid angle intervals is described. Dispersion measure - distance relations for radio pulsars based on this approach in the Galactic longitude and latitude intervals of Δl=0°±2° and Δb = 0°± 2° are displayed and comparisons are made with the predictions of the two commonly used models

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