robert buchler (38 Ergebnisse)

Zustand: Good. 237 pp., hardcover, ex library, else text clean & binding tight. - If you are reading this, this item is actually (physically) in our stock and ready for shipment once ordered. We are not bookjackers. Buyer is responsible for any additional duties, taxes, or fees required by recipient's country.

Hardcover. Zustand: Good. No Jacket. Missing dust jacket; Pages can have notes/highlighting. Spine may show signs of wear. ~ ThriftBooks: Read More, Spend Less 0.45.

Zustand: Good. Used book that is in clean, average condition without any missing pages.

Zustand: As New. Like New condition. Volume 848. (science, physics, astrophysics).

Zustand: very good. Gut/Very good: Buch bzw. Schutzumschlag mit wenigen Gebrauchsspuren an Einband, Schutzumschlag oder Seiten. / Describes a book or dust jacket that does show some signs of wear on either the binding, dust jacket or pages.

Zustand: Good. Former library book; may include library markings. Used book that is in clean, average condition without any missing pages.

Hardcover. Zustand: Very Good. pp.xvi, 326 pages, many figures in the text, a very good hardback (publisher's glazed cloth so no dust-jacket issued), ex-library [9027721254].

Soft cover. Zustand: Fine. No Jacket. 1st Edition. Fine in Softcover. 159pp 8vo. White spine with red titles.

Zustand: Very Good. Very Good condition. (Science, Mathematics, Physics).

Zustand: Very Good. Very Good condition. Volume 596. (Science, Physics).

Zustand: Very Good. Very Good condition. (Science, Physics, Astrophysics).

Zustand: New. pp. 155.

Hardcover. Zustand: Fine. pp.xvi, 326 pages, many figures in the text, a Fine hardback (publisher's laminated boards so no dust-jacket issued) [9027721254].

Hardcover. Zustand: Fine. No Jacket. Heavy book may require extra postage unless posted within South Africa. Publication of 178 pages. The Pictionary boards are in fine condition. Internally the pages are immaculately clean and complete. The binding is excellent. GK. Our orders are shipped using tracked courier delivery services.

Softcover. Zustand: Very Good. viii, 142pp. Pictorial light card covers. 8vo. Light chipping to edges and wear to covers. Internally, neat, clean, bright and tight.

8° (23,8 x 15,8 cm), Obrosch., 32 S., guter Zustand. 59 gr.

Trade paperback. Zustand: Very good. xi, [1], 155, [1] pages. Illustrations. References. Cover has slight wear and soiling. Published since 1823, the Annals of the New York Academy of Sciences (first published as the Annals of the Lyceum of Natural History of New York) is one of the oldest continuously published scientific serials in the United States. This issue devoted to Chaotic Phenomena in Astrophysics. Dr. Buchler was a professor emeritus of Physics at the University of Florida as the time of his 2012 death. Heinrich Karl Eichhorn (1927 - 1999) was a primary founder of modem astrometry and a man whose essential nature was innovation was lost with his passing . Heinz believed in a broad definition of astrometry, so as to include location and motion measured by any means, including radial velocities and interferometry; and his rigorous thinking was legendary among active astrometrists and students alike. Openness to the ideas of others and enthusiastic encouragement were major components of his image. 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". Founded on January 29, 1817, the New York Academy of Sciences was originally called the Lyceum of Natural History. Convened by the Academy's founder and first President, Samuel L. Mitchill, the first meeting of the Lyceum took place at the College of Physicians and Surgeons, located on Barclay Street near Broadway in lower Manhattan. The principal activities of the early Lyceum focused on hosting lectures, collecting natural history specimens, and establishing a library. 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. By 1826 the Lyceum owned "the richest collection of reptiles and fish in the country," however a fire in 1866 destroyed the collection completely. Following the fire, the Academy turned its focus away from collecting and instead to research, scientific publishing, and disseminating scientific information. From the outset, the New York Academy of Sciences membership was unique among scientific societies, with a democratic structure that allowed anyone to become a member, from laymen to respected professional scientists. For that reason, the membership has always included a mix of scientists, business people, academics, those working in government, and public citizens with an interest in science. Prominent members have included two United States Presidents Thomas Jefferson and James Monroe, as well as numerous well-known scientists such as Asa Gray (who served as the Superintendent of the Academy starting in 1836), John James Audubon, Alexander Graham Bell, Thomas Edison, Louis Pasteur, Charles Darwin, and Margaret Mead (who served for a time as the Vice President of the Academy). Prior to 1877, the Academy only admitted men, but on November 5, 1877, they elected Erminnie A. Smith the first female member. Membership has also included numerous Nobel Prize winners over the years. Early Academy members played prominent roles in the establishment of New York University in 1831 and the American Museum of Natural History in 1858. The Academy has made significant contributions to the scientific community 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; hosting an important gathering and publishing the first volume on the cardiovascular effects of smoking in 1960;[9] the founding of a Women in science.

Softcover. 155 S. Ehem. Bibliotheksexemplar mit Signatur und Stempel. GUTER Zustand, ein paar Gebrauchsspuren. Ex-library with stamp and library-signature. GOOD condition, some traces of use. D03751 897663896 Sprache: Englisch Gewicht in Gramm: 550.

Hardcover Aug 01, 1991. Zustand: gebraucht; gut. Kunstledereinband mit Goldprägung, minimalste Lagerspuren, Inhalt wie ungebraucht.

Paperback May 01, 1998. Zustand: gebraucht; wie neu.

Paperback. Zustand: Brand New. 1993 edition. 375 pages. 9.45x6.30x0.88 inches. In Stock.

kartoniert. Zustand: Sehr gut. Zust: Gutes Exemplar. 210 Seiten Englisch 300g.

(= Schriftenreihe des Slowakischen Matús Cernák-Instituts ; Nr. 7). 47 S. OBroschur. München, Johann Herp 1982.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The nonlinear theory of oscillating systems brings new aspects into the study of variable stars. Beyond the comparison of linear periods and the estimate of stability, the appearance and disappearance of possible modes can be studied in detail. While nonlinearity in stellar pulsations is not a very complicated concept, it generally requires extensive and sometimes so phisticated numerical studies. Therefore, the development of appropriate computational tools is required for applications of nonlinear theory to real phenomena in variable stars. Taking trends in variable star studies into consideration, the International Astronomical Union organized a colloquium for the nonlinear phenomena of variable stars at Mito, Japan in 1992. The colloquium served to give an overview of the new frontiers of variable star studies and to encourage further development of this field. The colloquium covered the fundamental theory, interesting observational facts, and the numerical modeling. The publication of the proceedings was somewhat delayed since one of the editors, M. T., was overwhelmed by administrative work. We are sorry that the excellent reviews of Drs. H. :Mori, M. Sano, and K. Makishima cannot be found in the proceedings. We also miss the summary given by Dr. W. W. Dziembowski. Throughout the editing procedure Dr. Y. Tanaka of Ibaraki University kindly helped us. Because of the unfortunate delay of the publication~ the significance of several papers may be affected. Even so, we believe that the papers are useful to variable star researchers because of their scientific importance.

Leinen in Folie. Zustand: Wie neu. 326 S. Ex-Library. Guter Zustand Ex-Library. ha1078106 Sprache: Englisch Gewicht in Gramm: 800.

Zustand: Sehr gut. Zustand: Sehr gut | Sprache: Englisch | Produktart: Bücher | Keine Beschreibung verfügbar.

Gebunden. Zustand: New. The nonlinear theory of oscillating systems has introduced new aspects to the study of variable stars. Beyond the comparison of linear periods and the estimate of stability, the appearance and disappearance of possible models can be studied in detail. While.

Hardcover. Zustand: Brand New. 388 pages. 10.00x6.50x1.25 inches. In Stock.

Softcover. Zustand: Very Good. 1991. An excellent copy, clean and unmarked throughout, some mild creasing along the spine but page edges crisp and no notable creases or wear. Covers firm and secure and similarly very well-presented with only minimal signs of prior shelving and storage. Why on Amazon do most sellers not describe their actual book? Buy with confidence and support a genuine Independent Bricks & Mortar Real Bookshop. We are Maynard & Bradley CAMBO & PBFA(now lapsed) members here in Leicester City Centre Size: 155 x 230 mm. 262. Item Type: Book. Quantity Available: 1. Shipped Weight: Under 500 grams. Category: Science & Technology; Britain/UK; 1990s; ISBN: 0897666674. ISBN/EAN: 9780897666671. Inventory No: 47720.

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The nonlinear theory of oscillating systems has introduced new aspects to the study of variable stars. Beyond the comparison of linear periods and the estimate of stability, the appearance and disappearance of possible models can be studied in detail. While nonlinearity in stellar pulsations is not a very complicated concept, it generally requires extensive and sometimes sophisticated numerical studies. The development of appropriate computational tools has allowed us to apply the nonlinear theory to real phenomena in variable stars. The International Astronomical Union Colloquium No. 134 presents a review of the new frontiers of variable star studies; one which will encourage further development of this field.