• Uma Kamboj
• Saqlain Bin Mushtaq
• Kiranjot Kaur
• Neha Munjal

A Neutron star is formed when an ordinary star dies -when a star has used almost every bit of its nuclear fuel it ceases to sustain itself, a point is reached when the thermal pressure produced in the core of star no longer exists therefore gravitational force exceeds the outward force of star due to which the star collapses, the new evolutionary species of star formed is called a Neutron star, and a rotating Neutron star is called a Pulsar. Study of pulsars have also been beneficial for time keeping as they are considered among the most accurate known natural time keepers. Therefore, we will study the formation and mechanisms related to Neutron stars specifically Pulsars. Consequently, leading to the interpretation of secondary data to study the properties such as time period, frequency and age of pulsars.

Timing analysis of Crab Pulsar using secondary data available at HEASARC

"Timing analysis of Crab Pulsar using secondary data available at HEASARC ", International Journal of Emerging Technologies and Innovative Research (www.jetir.org), ISSN:2349-5162, Vol.5, Issue 12, page no.271-280, December 2018, Available :http://www.jetir.org/papers/JETIREB06032.pdf

"Timing analysis of Crab Pulsar using secondary data available at HEASARC ", International Journal of Emerging Technologies and Innovative Research (www.jetir.org | UGC and issn Approved), ISSN:2349-5162, Vol.5, Issue 12, page no. pp271-280, December 2018, Available at : http://www.jetir.org/papers/JETIREB06032.pdf