Neutron Stars as a Source of the Short-Lived Nuclides in Ap-star Atmospheres

Details Neutron Stars as a Source of the Short-Lived Nuclides in Ap-star Atmospheres Neutron Stars as a Source of the Short-Lived Nuclides in Ap-star Atmospheres

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1016..460g&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From

Other

1

Neutron Stars, Pulsars, Polarons And Electron-Phonon Interactions, X- And Gamma-Ray Spectroscopy

Scientific paper

We propose a new explanation of some magnetic chemically peculiar (MCP) star anomalies, which is based on an assumption that such stars be the close binary systems with a secondary component being a neutron star. Within this hypothesis one can naturally explain the main anomalous features of MCP stars: first of all, an existence of the short-lived radioactive isotopes detected in some stars (like Przybylski's star (PS) and HR465), and some others peculiarities. Also we can assume the presence of the electron-positron annihilation emission lines (0.511 MeV) in the gamma spectrum of some MCP stars.

Affiliated with

Also associated with

No associations

Rating

Neutron Stars as a Source of the Short-Lived Nuclides in Ap-star Atmospheres does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Neutron Stars as a Source of the Short-Lived Nuclides in Ap-star Atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutron Stars as a Source of the Short-Lived Nuclides in Ap-star Atmospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1406432