mestel leon (43 resultados)

Condición: Good. Volume 99. This is an ex-library book and may have the usual library/used-book markings inside.This book has hardback covers. In good all round condition. No dust jacket. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,1450grams, ISBN:0198517610.

Condición: Good. Volume 99. This is an ex-library book and may have the usual library/used-book markings inside.This book has hardback covers. In good all round condition. No dust jacket. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,1450grams, ISBN:9780198517610.

Condición: Good. Volume 99. This is an ex-library book and may have the usual library/used-book markings inside.This book has hardback covers. In good all round condition. No dust jacket. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,1450grams, ISBN:9780198517610.

Condición: Gut. Formateinband: Broschierte Ausgabe XIV, 837 S. (23 cm) Paperback-Edition; 1. Aufl.; Außen etwas gealtert; sonst gut und textsauber erhalten. Sprache: Englisch Gewicht in Gramm: 1400 [Stichwörter: Astrophysik, Kosmologie, Symposium].

Mar 01, 1992. Condición: gebraucht; gut. Einband mit kleiner Kuli Markierung, Inhalt wie ungebraucht.

Gr.-8°, original softcover. 1. ed. With numerous images, XX, 636 p. Shelfmark on spine, stamp on preliminary page and title, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.

kartoniert kartoniert. Condición: Sehr gut. 840 Seiten Zust: Gutes Exemplar. Schneller Versand und persönlicher Service - jedes Buch händisch geprüft und beschrieben - aus unserem Familienbetrieb seit über 25 Jahren. Eine Rechnung mit ausgewiesener Mehrwertsteuer liegt jeder unserer Lieferungen bei. Wir versenden mit der deutschen Post. Sprache: Englisch Gewicht in Gramm: 1140.

Hard Cover. Condición: Very Good. First Edition. VERY GOOD; FIRST EDITION; EX-LIBRARY; although it is an ex-library the pages inside are clean and unmarked and the binding is tight; there are only a few stamps of library origin inside; all other labels have been removed; a nice copy; Size: 8vo - over 7¾" - 9¾" tall. Ex-Library.

Condición: New. pp. 754 Index 2nd Edition.

Condición: New. pp. 754.

Condición: New. pp. 754.

Condición: New. pp. 658.

Condición: New.

Condición: New.

Condición: As New. Unread book in perfect condition.

Condición: As New. Unread book in perfect condition.

Hardcover. Condición: Near Fine. Estado de la sobrecubierta: Near Fine. 1st Edition. 258 Pp. Orange Cloth Stamped In Black. First Printing. Near Fine In Near Fine Dust Jacket, No Marks. Thorne's Article, With A Lengthy Bibliography, Is An Expanded Version Of His 1975 Chicago Lecture.

Condición: New.

Condición: New. In.

Condición: New.

Condición: As New. Unread book in perfect condition.

Condición: As New. Unread book in perfect condition.

Condición: New. Stellar magnetism is the study of the magnetic field of the Sun and other stars. This book is an authoritative account with astronomical scope. Most of the important topics are treated in mathematical depth with references to other relevant literature. Series: International Series of Monographs on Physics. Num Pages: 656 pages, 3 plates, 3 halftones, 120 line figures. BIC Classification: PGM; PHFP; PHK; PHVB. Category: (P) Professional & Vocational. Dimension: 243 x 165 x 38. Weight in Grams: 1357. . 1999. Hardback. . . . .

Hardback. Condición: New. Most stars appear to show some degree of magnetic activity. Varying magnetic fields show up in the familiar sun-spot cycle and in similar activity in other cool stars. Many hot stars carry steady magnetic fields stronger than the average solar field and are well described as oblique rotators. A similar model is applicable to the rapidly rotating, enormously dense neutron stars with their far stronger fields, observed as radio and X-ray pulsars. Galactic magnetic fields may play a crucial role in star formation, and in the spectacular behaviour in galactic nuclei. Cosmical magnetism in general is a rapidly developing field, and this book has grown out of the lifelong work of an outstanding researcher in the area. An authoritative account with broad astronomical scope, its thorough, careful and well-argued approach makes it a fine addition to the professional literature. Most of the important topics are treated in mathematical depth with references to other relevant literature. Some of the studies, especially those on accretion discs, dynamos, and winds, are applicable to galaxies and galactic nuclei. This book is sure to become an invaluable professional reference and guide to current thinking in the field. It will be of particular interest to graduate students, for whom it shows how the area has developed and indicates the many challenging research problems, some of which may soon yield their secrets to the emerging supercomputers.

Hardcover. Condición: new. Hardcover. Most stars appear to show some degree of magnetic activity. Varying magnetic fields show up in the familiar sun-spot cycle and in similar activity in other cool stars. Many hot stars carry steady magnetic fields stronger than the average solar field and are well described as oblique rotators. A similar model is applicable to the rapidly rotating, enormously dense neutron stars with their far stronger fields, observed as radio and X-ray pulsars. Galactic magneticfields may play a crucial role in star formation, and in the spectacular behaviour in galactic nuclei. Cosmical magnetism in general is a rapidly developing field, and this book has grown out of thelifelong work of an outstanding researcher in the area. An authoritative account with broad astronomical scope, its thorough, careful and well-argued approach makes it a fine addition to the professional literature. Most of the important topics are treated in mathematical depth with references to other relevant literature. Some of the studies, especially those on accretion discs, dynamos, and winds, are applicable to galaxies and galactic nuclei. This book is sure to become an invaluableprofessional reference and guide to current thinking in the field. It will be of particular interest to graduate students, for whom it shows how the area has developed and indicates the many challengingresearch problems, some of which may soon yield their secrets to the emerging supercomputers. Stellar magnetism is the study of the magnetic field of the Sun and other stars and is a rapidly developing field of astrophysics. This book has grown out of the lifelong work of an outstanding researcher in the subject. It is an authoritative account with broad astronomical scope, and its thorough, careful, and well-argued approach makes it a fine addition to the professional literature. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.

Condición: New. Stellar magnetism is the study of the magnetic field of the Sun and other stars. This book is an authoritative account with astronomical scope. Most of the important topics are treated in mathematical depth with references to other relevant literature. Series: International Series of Monographs on Physics. Num Pages: 656 pages, 3 plates, 3 halftones, 120 line figures. BIC Classification: PGM; PHFP; PHK; PHVB. Category: (P) Professional & Vocational. Dimension: 243 x 165 x 38. Weight in Grams: 1357. . 1999. Hardback. . . . . Books ship from the US and Ireland.

Hardback. Condición: New. Most stars appear to show some degree of magnetic activity. Varying magnetic fields show up in the familiar sun-spot cycle and in similar activity in other cool stars. Many hot stars carry steady magnetic fields stronger than the average solar field and are well described as oblique rotators. A similar model is applicable to the rapidly rotating, enormously dense neutron stars with their far stronger fields, observed as radio and X-ray pulsars. Galactic magnetic fields may play a crucial role in star formation, and in the spectacular behaviour in galactic nuclei. Cosmical magnetism in general is a rapidly developing field, and this book has grown out of the lifelong work of an outstanding researcher in the area. An authoritative account with broad astronomical scope, its thorough, careful and well-argued approach makes it a fine addition to the professional literature. Most of the important topics are treated in mathematical depth with references to other relevant literature. Some of the studies, especially those on accretion discs, dynamos, and winds, are applicable to galaxies and galactic nuclei. This book is sure to become an invaluable professional reference and guide to current thinking in the field. It will be of particular interest to graduate students, for whom it shows how the area has developed and indicates the many challenging research problems, some of which may soon yield their secrets to the emerging supercomputers.

Trade paperback. Condición: Good. Presumed First Edition, First printing. xiv, 840, [2] pages. Figures. Tables. References. List of Poster Papers. Index of Contributors. Cover has some wear and soiling. "Papers . presented at the combined Fifteenth Texas Symposium and the Fourth ESO-CERN Symposium, which was held on December 16-21, 1990, in Brighton, U.K." The five mornings were devoted to plenary lectures and the four afternoons to three parallel minisymposia on neutron star and black hole astrophysics, particles astronomy--status and prospects, and large-scale structure and galaxy formation. There was also a minisymposium held over two evening sessions on space-based and lunar-based astrophysics. On the evening of Tuesday, December 18, 1990 Dr. Stephen Hawking gave an open lecture on "The Beginning of the Universe" (pages 315-322). The New York Academy of Sciences (originally the Lyceum of Natural History) was founded in January 1817. It is one of the oldest scientific societies in the United States. An independent, non-profit organization with more than 20,000 members in 100 countries, the Academy's mission is "to advance scientific research and knowledge; to support scientific literacy; and to promote the resolution of society's global challenges through science-based solutions". In 1823, the Lyceum began publishing its own scientific journal, then the Annals of the Lyceum of Natural History of New York, now the Annals of the New York Academy of Sciences. The Academy has made significant contributions to science during the course of its history, including publishing one of the first studies on environmental pollution in 1876; conducting a scientific survey of Puerto Rico from 1907-1934; the first conference on antibiotics on 21 July 1948; publishing the first volume on the cardiovascular effects of smoking in 1960; the founding of a Women in science Committee in 1977; the world's first major scientific conference on AIDS in 1983; and a conference on SARS in 2003.

Condición: new. Questo è un articolo print on demand.

Condición: new. Questo è un articolo print on demand.