An incomparable reference for astrophysicists studying pulsars and other kinds of neutron stars, Theory of Neutron Star Magnetospheres sums up two decades of astrophysical research. It provides in one volume the most important findings to date on this topic, essential to astrophysicists faced with a huge and widely scattered literature. F. Curtis Michel, who was among the first theorists to propose a neutron star model for radio pulsars, analyzes competing models of pulsars, radio emission models, winds and jets from pulsars, pulsating X-ray sources, gamma-ray burst sources, and other neutron-star driven phenomena. Although the book places primary emphasis on theoretical essentials, it also provides a considerable introduction to the observational data and its organization. Michel emphasizes the problems and uncertainties that have arisen in the research as well as the considerable progress that has been made to date.
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Descrizione libro U.S.A.: University of Chicago Press, 1990. Hardcover. Condizione libro: As New. No Jacket. 1st Edition. NOT ex-library copy; no dustjacket issued. Codice libro della libreria ABE-16343505940
Descrizione libro University of Chicago Press, 1991, 1991. Hardcover. Condizione libro: VG. Condizione sovraccoperta: None. First Edition. 8vo - over 7¾" - 9¾" tall. VG/None. First Edition. 8vo - over 7¾" - 9¾" tall. 517 pp, hardbound, 1st printing, superficial dampstaining and soiling to 1" of foredge of front board, otherwise this copy would be "F-," super clean, binding tight, spine titling bright and no markings, NOT EXLIB. Codice libro della libreria 5056
Descrizione libro University of Chicago Press, 1990. Hardcover. Condizione libro: Good. Codice libro della libreria mon0001454198