'Binary pulsars' presentation slideshows

Fundamental Physics and Astrophysics using Pulsars and the SKA

612 views • 51 slides

Stellar Evolution after the Main Sequence

Stellar Evolution after the Main Sequence. High Mass Stars. 1000. 100. 10. 1. .1. .01. The Path to the Main Sequence. O B A F G K M. After the Main Sequence.

647 views • 47 slides

Searching for Radio Pulsars

322 views • 19 slides

He star evolutionary channel to intermediate-mass binary pulsars with a short-orbital-period

He star evolutionary channel to intermediate-mass binary pulsars with a short-orbital-period. Chen Wen-Cong. School of Physics, Peking University Department of Physics, Shangqiu Normal University. Normal Radio Pulsars and Millisecond pulsars. Normal radio pulsars. MSPs.

254 views • 13 slides

ASTRONOMY

ASTRONOMY. Chapter 30 Pulsars and Neutron Stars. Formation of a Neutron Star. In the iron core of a high-mass star: Iron nuclei break into He nuclei, protons, and neutrons Energy is carried out and the pressure drops The core collapses.

207 views • 10 slides