Next: Other parameters of the Up: The Model Previous: Initial binary parameters . As we only deal with initially massive binary systems (their primary's mass is higher than 10 ), which are capable of evolving off the main sequence during less than years, the compact stars left behind stellar evolution are (in the case of the most massive stars) NSs and BHs. ... For a NS belonging to a binary, the evolution complicates as the secondary star evolves: for example, (recycling), etc. ...

... The last stand before MAP: cosmological parameters from lensing, CMB and galaxy clustering" astro-ph/0212417 . ... Скопления галактик: J. Patrick Henry "Evolution of the X-ray Properties of Clusters of Galaxies" astro-ph/0207148 . ... Supernova Explosions and Neutron Star Formation" astro-ph/0103015 . ... Рентгеновские источники в шаровых скоплениях: Frank Verbunt "Binary evolution and neutron stars in globular clusters" astro-ph/0210057 . ... Neutrino Emission from Neutron Stars" astro-ph/0012122 ....

... SGML . The text/html content type . In this section, we begin the specification of HTML 4.0, starting with the contract between authors, documents, users, and user agents. ... These recommendations are not normative and conformance with this specification does not depend on their realization. ... An HTML document is an SGML document that meets the constraints of this specification. ... A user is a person who interacts with a user agent to view, hear, or otherwise use a rendered HTML document. ...