Studies of accreting and non-accreting neutron stars

Authors	G.M. Stollman
Supervisors	E.P.J. van den Heuvel
Cosupervisors	J.A. van Paradijs
Award date	15-04-1987
Organisations	Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Document type	PhD thesis
Note	Research conducted at: Universiteit van Amsterdam
Downloads	Thesis Cover Titlepage CONTENTS INTRODUCTION AND SUMMARY PART A STATISTICAL STUDIES OF RADIO PULSARS CHAPTER I DOES A CORRELATION BETWEEN THE MAGNETIC FIELD AND THE TRANSVERSE VELOCITY EXIST FOR RADIO PULSARS? CHAPTER II A POSSIBLE DISCRIMINATION BETWEEN TWO LUMINOSITY LAWS FOR RADIO PULSARS CHAPTER III THE RADIO LUMINOSITY OF PULSARS CHAPTER IV PULSAR STATISTICS PART B QUASI-PERIODIC OSCILLATIONS IN LOW-MASS X-RAY BINARIES CHAPTER V TRYING TO UNDERSTAND QPO: A REVIEW CHAPTER VI A QUALITATIVE MODEL FOR GX 5-1 CHAPTER VII BIMODAL ACCRETION IN GX5-1 AND A POSSIBLE CONSTRAINT ON ITS ROTATION PERIOD CHAPTER VIII COUPLING OF AN ACCRETION DISK CORONA WITH A WEAKLY MAGNETIC NEUTRON STAR AND A POSSIBLE RELATION WITH QPO. PART C THE PROBLEM OF SUPER-EDDINGTON LUMINOSITIES IN X-RAY BURST SOURCES CHAPTER IX SUPER-EDDINGTON LUMINOSITIES IN X-RAY BURSTS CHAPTER X SUPER-EDDINGTON FLUXES IN A QUASI-HYDROSTATIC, OPTICALLY THICK REGION OF A NEUTRON-STAR OUTER ENVELOPE. SAMENVATTING NAWOORD CURRICULUM VITAE STELLINGEN behorende bij het proefschrift Cover
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