|
|
|||
|
||||
OverviewIn X-ray binaries, neutron stars (the very dense stellar remnants of heavy stars) accrete matter from a close-by companion star. This matter eventually falls on the neutron star, significantly affecting it. I.e., the star is spun up to very high spin rates. In the end, it might rotate 1000 times a second which causes very fast oscillations in its X-ray brightness. This workshop was to celebrate the 10th anniversary of the discovery of the first system in which this signal was found and discuss the most recent observational and theoretical insight in the nature of these systems. Full Product DetailsAuthor: Rudy Wijnands , Diego Altamirano , Paolo Soleri , Nathalie DegenaarPublisher: American Institute of Physics Imprint: American Institute of Physics Volume: No. 1068 Dimensions: Width: 15.60cm , Height: 1.50cm , Length: 23.40cm Weight: 0.553kg ISBN: 9780735405998ISBN 10: 0735405999 Pages: 268 Publication Date: 01 December 2008 Audience: Professional and scholarly , Professional & Vocational Format: Hardback Publisher's Status: Unknown Availability: In Print Limited stock is available. It will be ordered for you and shipped pending supplier's limited stock. Table of ContentsReviewsAuthor InformationTab Content 6Author Website:Countries AvailableAll regions |
||||