A red Giant Star With a Strange Star as a Core

Details A red Giant Star With a Strange Star as a Core A red Giant Star With a Strange Star as a Core

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.243h&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

The model of a red giant with the mass 5Modot, luminosity % 41740Lodot and the radius 980Rodot and with the strange quark as a core has been constructed. A comparison has been made with the object of Thorne-Zytkow that has analogous integral parameters. The difference in the inner structure is manifested just at the dense core. Convection does not stop up to the strange star, the matter over the core is withstood only due to the emission from the strange star. The lifetime of the red giants with the strange star turns out to be 500 times shorter than that of the Thorne-Zytkow's object, and is 10^5 year order.

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