71 books for « oppenheimer j r »Edit

‎Forces in molecules [Feynman] (+) The mechanism of nuclear fission [N. Bohr. & J. A. Wheeler] ""On continued gravitational contraction"" [J. R. Oppenheimer & H. Snyder]. - [FEYNMAN'S UNDERGRADUATE THESIS & THE FIRST THEORETICAL DESCRIPTION OF A SINGULARITY]‎

‎[Lancaster], American Institute of Physics, 1939. Royal8vo. Bound in contemporary full red cloth with gilt lettering to spine. Entire volume of ""The Physical Review"", Volume 56, Second Series, July 1 - December 15, 1939. ""Development Department"" in small gilt lettering to lower part of spine. A very fine and clean copy. [Feynman:] Pp. 340-43. [Bohr & Wheeler:] Pp. 426-50. [Oppenheimer & Snyder:] Pp. 455-59. [Entire volume: X, 1264 pp.].‎

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‎First printing of three landmark papers, all of seminal importance in history of physics: Feynman's undergraduate thesis at MIT, the intricacies of the fission process, the groundwork for atomic and hydrogen bombs and the forgotten birth of black holes: The first theoretical description of a black hole, the production of a singularity when a sufficiently large neutron star collapses.First printing of ""FORCES IN MOLECULES"" - know known as Feynman-Hellmann theorem - is Feynman's undergraduate thesis at MIT, published when he was just twenty-one, which helped to establish his name in the world of physics. ""This work treated the problem of molecular forces from a thoroughly quantum-mechanical point of view, arriving at a simple means of calculating the energy of a molecular system that continues to guide quantum chemists."" (DSB). ""As Feynman conceived the structure of molecules, forces were the natural ingredients. He saw springlike bonds with varying stiffness, atoms attracting and repelling one another. The usual energy-accounting methods seemed secondhand and euphemistic: [He demonstrated that] the force on an atom's nucleus is no more or less than the electrical force from the surrounding field of charged electrons-the electrostatic force. Once the distribution of charge has been calculated quantum mechanically, then from that point forward quantum mechanics disappears from the picture. The problem becomes classical"" the nuclei can be treated as static points of mass and charge. Feynman's approach applies to all chemical bonds"" (Gleick, The Life and Science of Richard Feynman, P. 54).Oppenheimer and Snyder's ""ON CONTINUED GRAVITATIONAL CONTRACTION"" constitute the very first theoretical prediction of a singularity when a sufficiently large neutron star collapses. This phenomenon was later to be coined as a black hole. ""Had J. Robert Oppenheimer not led the US effort to build the atomic bomb, he might still have been remembered for figuring out how a black hole could form."" (American Physical Society). The paper has by several physics historians been described as the forgotten birth of black holes. ""Oppenheimer and his graduate student George Volkoff presented the first analysis of the formation of a neutron star in a 1939 Physical Review paper titled, ""On Massive Neutron Stars"". Oppenheimer wondered what would happen to a very massive neutron star. The Schwartzschild analysis of General Relativity has a theoretical limit, called the ""Schwartzschild limit"", when the ratio of mass-to-radius of a star is 236,000 times greater than the ratio for our sun. When this limit is exceeded, the Schwartzschild analysis does not yield a solution. Oppenheimer believed that a neutron star could have sufficient mass to exceed this limit. What would happen to it? Oppenheimer and his graduate student Hartland Snyder applied General Relativity theory to a star with sufficient mass and density to exceed the Schwartzschild limit. The Schwartzschild analysis assumed that the size of the star stays constant with time. Oppenheimer and Snyder found that they could achieve a real solution from General Relativity when the Schwartzschild limit is exceeded by assuming that the diameter of the star decreases with time. They presented their analysis in a 1939 Physical Review paper, titled, ""On Continual Gravitational Contraction,"" which concluded with: ""When all thermonuclear sources of energy are exhausted, a sufficiently heavy star will collapse. Unless fission due to rotation, the radiation of mass, or the blowing off of mass by radiation, reduce the star's mass to the order of that of the sun, this contraction will continue indefinitely."" This analysis concluded that when the Schwartzschild limit is exceeded, the star must collapse indefinitely until it reaches a singularity having an infinite density of matter"" (Bjornson, Singularity Predictions of General Relativity, P. 4).The Chandrasekhar / Eddington controvery in the mid 30ies did discuss the fate of neutron stars but the first thoroughly theoretical desciption was first published here. ""THE MECHANISM OF NUCLEAR FISSION"" is the first fully worked out theory of nuclear fission, which laid the groundwork for atomic and hydrogen bombs.""Wheeler's technical mastery of physics is best seen in the classic paper of Bohr and Wheeler. Bohr and Wheeler wrote the paper in Princeton, where Bohr was visiting in the spring of 1939, a few months after the discovery of fission. The paper is a masterpiece of clear thinking and lucid writing. It reveals, at the center of the mystery of fission, a tiny world where everything can be calculated and everything understood. The tiny world is a nucleus of uranium 236, formed when a neutron is freshly captured by a nucleus of uranium 235. The uranium 236 nucleus sits precisely on the border between classical and quantum physics. Seen from the classical point of view, it is a liquid drop composed of a positively charged fluid. The electrostatic force that is trying to split it apart is balanced by the nuclear surface tension that is holding it together. The energy supplied by the captured neutron causes the drop to oscillate in various normal modes that can be calculated classically. Seen from the quantum point of view, the nucleus is a superposition of a variety of quantum states leading to different final outcomes. The final outcome may be a uranium 235 nucleus with a re-emitted neutron, or a uranium 236 nucleus with an emitted gamma-ray, or a pair of fission-fragment nuclei with one or more free neutrons. Bohr and Wheeler calculate the cross-section for fission of uranium 235 by a slow neutron and get the right answer within a factor of two. Their calculation is a marvelous demonstration of the power of classical mechanics and quantum mechanics working together. By studying this process in detail, they show how the complementary views provided by classical and quantum pictures are both essential to the understanding of nature. Without the combined power of classical and quantum concepts, the intricacies of the fission process could never have been understood. Bohr's notion of complementarity is triumphantly vindicated"" (John Archibald Wheeler, Proceedings of the American Philosophical Society 154 (2010)).‎

‎The mechanism of nuclear fission [N. Bohr. & J. A. Wheeler] ""On continued gravitational contraction"" [J. R. Oppenheimer & H. Snyder]. - [THE FIRST THEORETICAL DESCRIPTION OF A SINGULARITY]‎

‎Lancaster, American Institute of Physics, 1939. Royal8vo. In the original green printed wrappers. In ""The Physical Review"", Volume 56, Second Series, Number 5, September 1. With cloth back-strip. A quire, affecting both papers, detached but without any loss of paper. A few minor tear throughout, far from affecting text. [Bohr & Wheeler:] Pp. 426-50. [Oppenheimer & Snyder:] Pp. 455-59. [Entire volume: Pp. 387-486].‎

‎First printing of two landmark papers, all of seminal importance in history of physics: The intricacies of the fission process, the groundwork for atomic and hydrogen bombs and the forgotten birth of black holes: The first theoretical description of a black hole, the production of a singularity when a sufficiently large neutron star collapses.Oppenheimer and Snyder's ""ON CONTINUED GRAVITATIONAL CONTRACTION"" constitute the very first theoretical prediction of a singularity when a sufficiently large neutron star collapses. This phenomenon was later to be coined as a black hole. ""Had J. Robert Oppenheimer not led the US effort to build the atomic bomb, he might still have been remembered for figuring out how a black hole could form."" (American Physical Society). The paper has by several physics historians been described as the forgotten birth of black holes. ""Oppenheimer and his graduate student George Volkoff presented the first analysis of the formation of a neutron star in a 1939 Physical Review paper titled, ""On Massive Neutron Stars"". Oppenheimer wondered what would happen to a very massive neutron star. The Schwartzschild analysis of General Relativity has a theoretical limit, called the ""Schwartzschild limit"", when the ratio of mass-to-radius of a star is 236,000 times greater than the ratio for our sun. When this limit is exceeded, the Schwartzschild analysis does not yield a solution. Oppenheimer believed that a neutron star could have sufficient mass to exceed this limit. What would happen to it? Oppenheimer and his graduate student Hartland Snyder applied General Relativity theory to a star with sufficient mass and density to exceed the Schwartzschild limit. The Schwartzschild analysis assumed that the size of the star stays constant with time. Oppenheimer and Snyder found that they could achieve a real solution from General Relativity when the Schwartzschild limit is exceeded by assuming that the diameter of the star decreases with time. They presented their analysis in a 1939 Physical Review paper, titled, ""On Continual Gravitational Contraction,"" which concluded with: ""When all thermonuclear sources of energy are exhausted, a sufficiently heavy star will collapse. Unless fission due to rotation, the radiation of mass, or the blowing off of mass by radiation, reduce the star's mass to the order of that of the sun, this contraction will continue indefinitely."" This analysis concluded that when the Schwartzschild limit is exceeded, the star must collapse indefinitely until it reaches a singularity having an infinite density of matter"" (Bjornson, Singularity Predictions of General Relativity, P. 4).The Chandrasekhar / Eddington controvery in the mid 30ies did discuss the fate of neutron stars but the first thoroughly theoretical desciption was first published here. ""THE MECHANISM OF NUCLEAR FISSION"" is the first fully worked out theory of nuclear fission, which laid the groundwork for atomic and hydrogen bombs.""Wheeler's technical mastery of physics is best seen in the classic paper of Bohr and Wheeler. Bohr and Wheeler wrote the paper in Princeton, where Bohr was visiting in the spring of 1939, a few months after the discovery of fission. The paper is a masterpiece of clear thinking and lucid writing. It reveals, at the center of the mystery of fission, a tiny world where everything can be calculated and everything understood. The tiny world is a nucleus of uranium 236, formed when a neutron is freshly captured by a nucleus of uranium 235. The uranium 236 nucleus sits precisely on the border between classical and quantum physics. Seen from the classical point of view, it is a liquid drop composed of a positively charged fluid. The electrostatic force that is trying to split it apart is balanced by the nuclear surface tension that is holding it together. The energy supplied by the captured neutron causes the drop to oscillate in various normal modes that can be calculated classically. Seen from the quantum point of view, the nucleus is a superposition of a variety of quantum states leading to different final outcomes. The final outcome may be a uranium 235 nucleus with a re-emitted neutron, or a uranium 236 nucleus with an emitted gamma-ray, or a pair of fission-fragment nuclei with one or more free neutrons. Bohr and Wheeler calculate the cross-section for fission of uranium 235 by a slow neutron and get the right answer within a factor of two. Their calculation is a marvelous demonstration of the power of classical mechanics and quantum mechanics working together. By studying this process in detail, they show how the complementary views provided by classical and quantum pictures are both essential to the understanding of nature. Without the combined power of classical and quantum concepts, the intricacies of the fission process could never have been understood. Bohr's notion of complementarity is triumphantly vindicated"" (John Archibald Wheeler, Proceedings of the American Philosophical Society 154 (2010)).‎

‎Note on the Transmutation Function for Deutrons. [In ""The Physical Review, Volume 48, Second Series, Number 6, September, 1935]. - [FIRST PUBLICATION OF THE OPPENHEIMER-PHILLIPS PROCESS]‎

‎Lancaster, American Physical Society, 1935. Lex8vo. Entire volume in the original printed blue/grey wrappers. Minor miscolouring and soiling to extremities. A fine and clean copy. Pp. 500-2. [Entire issue: Pp. 491-572].‎

‎First printing of this important paper in which the Oppenheimer-Phillips process was presented for the first time - Oppenheimer's ""most important contribution in this area"" (Oppenheimer. A Life. P. 29).A deuteron, entering a heavy nucleus, is split into proton plus neutron, one of these particles being retained by the nucleus while the other is re-emitted. After the second world war this became a fundamental tool in the study of nuclear energy levels and their properties. Phillips was Oppenheimer's research associate in 1933-4.In ""The Physical Review - The First Hundred Years. A Selection of Seminal Papers and Commentaries"".‎

‎Energy Production in Stars (+) On Massive Neutron Cores (+) Neutron Stars and the Tolman-Oppenheimer-Volkov Limit. - [HANS BETHE'S NOBEL PRIZE WINNING PAPER AND GENERAL RELATIVISTIC THEORY OF STELLAR STRUCTURE]‎

‎[Lancaster], American Institute of Physics, 1939. Royal8vo. Bound in contemporary full red cloth with gilt lettering to spine. Entire volume of ""The Physical Review"", Volume 55, Second Series, January 1 - June 15, 1939. ""Development Department"" in small gilt lettering to lower part of spine. A very fine and clean copy. [Bethe:] Pp. 434-456. [Oppenheimer & Volkoff:] Pp. 374-381. [Entire volume: 1300 pp.].‎

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‎First printing of ""ENERGY PRODUCTION IN STARS"", Hans Bethe's seminal Nobel Prize winning paper on neucleosynthesis. It was the first time an astrophysical subject was recognized by the Nobel Committee. Bethe's work on nuclear reactions led him to discover the reactions that supply the energy in stars. In this paper, Bethe shows that ""the most important source of energy in ordinary stars is the reactions of carbon and nitrogen with protons"" (Bethe, Energy Production in Stars). Bethe began by analyzing the different possibilities for reactions by which hydrogen is fused into helium. He showed two processes to be the sources of energy generation capable of keeping stars hot. The first, the proton-proton chain, is the dominant energy source in stars with masses up to about the mass of the Sun. The second, the carbon-nitrogen-oxygen cycle, is the most important in more massive stars. ""ON MASSIVE NEUTRON CORES"" and NEUTRON STARS AND THE TOLMAN-OPPENHEIMER-VOLKOV LIMIT, two landmark papers which ""for the first time laid a general relativistic theory of stellar structure"" (Pais, Subtle is the Lord), thereby proving Einstein wrong in his conclusion that no star could collapse indefinitely.In the paper they addressed the question that Landau's paper, and also Oppenheimer and Serber's, had failed to consider: what is the maximum mass for stable neutron-star? This paper applied Tolman's method to calculate the gravitational equilibrium of a neutron star and predict the conditions under which it will continue collapsing into a black hole (the Tolman-Oppenheimer-Volkov Limit). The issue contain several other papers of interest: 1. Tolman, Richard. ""Static Solutions of Einstein's Field Equations for Spheres of Fluid"" - This paper developed a method for applying Einstein's field equations to static spheres of fluid in such a manner as to facilitate the development of exact solutions using known analytic functions)"" Jenkins and Segre's ""Quadratic Zeeman Effect"" and ""Zeeman Effect of the Forbidden Lines of Potassium"" .2. Gamow & Teller. ""On the Origin of Great Nebulae"". 3. Seaborg & Segre. ""Nuclear Isomerism in Element 43"" 4. Gentner & Segre. ""Appendix on the Calibration of the Ionization Chamber"". 5. Bethe. ""On the Absence of Polarization in Electron Scattering"" & ""Meson Theory of Nuclear Forces.""‎

‎Über die Strahlung der freien Elektronen im Coulombfeld.‎

‎Berlin, Springer, 1929. 8vo. Bound in contemporary half cloth with gilt lettering, In ""Zeitschrift für Physik"", Band 55, 1929. Entire issue offered. Two stamps to title page, otherwise fine. Pp. 725-737. [Entire volume: VI, 821 pp].‎

‎First appearance of Oppenheimer's paper on the radiation of free electrons in the Coulomb field.Oppenheimer is primarily known for his role as the scientific director of the Manhattan Project and is often referred to as the father of the atomic bomb. In 1947, Oppenheimer accepted an offer from to take up the directorship of the Institute for Advanced Study in Princeton, New Jersey, where he held Einstein's old position of Senior Professor of Theoretical Physics. ‎

‎Über die Strahlung der freien Elektronen im Coulombfeld.‎

‎Berlin, Springer, 1929. 8vo. Bound in contemporary half cloth with gilt lettering, In ""Zeitschrift für Physik"", Band 55, 1929. Entire volume offered. Two stamps to title page, otherwise fine. Pp. 725-737. [Entire volume: VI, 821 pp].‎

‎First appearance of Oppenheimer's paper on the radiation of free electrons in the Coulomb field.Oppenheimer is primarily known for his role as the scientific director of the Manhattan Project and is often referred to as the father of the atomic bomb. In 1947, Oppenheimer accepted an offer from to take up the directorship of the Institute for Advanced Study in Princeton, New Jersey, where he held Einstein's old position of Senior Professor of Theoretical Physics. ‎

‎Zur Quantentheorie der Molekeln. - [THE BORN-OPPENHEIMER APPROXIMATION]‎

‎Leipzig, Ambrosius Barth, 1927. 8vo. In contemporary full cloth with gilt lettering to spine. In ""Annalen der Physik"", Vierte Folge, Band 84. Entire volume offered. Library labels pasted on the pasted down front free end paper. Traces after a label to lower part of spine. Stamp to title page. Internally fine and clean. Pp. 457-484. [Entire volume: 1080, VIII pp.].‎

‎First printing of Born and Oppenheimer's famous paper in which the Born-Oppenheimer approximation which is the computation of the energy and the wavefunction of an average-size molecule. It is still an indispensable part of quantum chemistry today.‎

‎Oppenheimer F. Oetinger J. Collective and private land ownership Practical be‎

‎Oppenheimer F. Oetinger J. Collective and private land ownership Practical be. Library of the Jewish National Foundation. M. Publication of the Central Office of the Jewish National Foundation in The Hague. 1917. VIII and 72 p. SKUalb422cbf0dcd12f6c7.‎

‎Historical Studies in the Physical Sciences - Volume 12, Part 2 (1982) , (In the matter of J. Robert Oppenheimer - Werner Siemens and the origin of the Physikalisch - Technische Reichsanstalt, 1872-1887 - Theoretical predispositions in experimental physics : Einstein and the gyromagnetic experiments, 1915-1925 - Experimentalists among the mathematicians : Physics in the Cambridge Natural Sciences Tripos, 1851 - 1900 - Audacious enterprise : The Einsteins and electrotechnology in late nineteenth-century Munich)‎

‎University of California Press, History of Science and Technology , Historical Studies in the Physical Sciences Malicorne sur Sarthe, 72, Pays de la Loire, France 1982 Book condition, Etat : Bon paperback, editor's white wrappers, title in blue grand In-8 1 vol. - 197 pages‎

‎few black and white illustrations and text-figures 1st edition, 1982 "Contents, Chapitres : Barton J. Bernstein : "" In the matter of J. Robert Oppenheimer"" - David Cahan : Werner Siemens and the origin of the Physikalisch - Technische Reichsanstalt, 1872-1870 - Peter Galison : Theoretical predispositions in experimental physics : Einstein and the gyromagnetic experiments, 1915- 1925 - David B. Wilson : Experimentalists among the mathematicians : Physics in the cambridge Natural Sciences Tripos, 1851 - 1900 - Lewis Pyenson : Audacious enterprise : The Einsteins and electrotechnology in late nineteenth-century Munich" plastified wrappers, transparent, else near fine, no markings - pages 196 to 392‎

‎Oppenheimer et la bombe atomique.‎

‎ Seghers, coll. "Savants du monde entier" n° 7 1962 1 vol. broché in-8 carré, broché, couverture illustrée d'un portrait, 223 pp., 12 planches hors-texte. En belle condition.‎

‎Sans totem ni tabou‎

‎Ramsay Broché D'occasion bon état 20/03/2017 240 pages ‎

‎Max Oppenheimer. Verzeichnis der Druckgrafik.‎

‎München, Galerie Michael Pabst, 1993, 4° (29,5 x 21 cm), 30 Bll. mit vielen z. T. farbigen ganzseitigen Abbildungen, OBroschur mit farbiger Deckelillustration. ‎

‎Verzeichnet 72 Radierungen, 28 Lithographien und 4 Holzschnitte. Mit der Preisliste der Galerie. Sauberes, gut erhaltenes Exemplar. ‎

‎BIG EGO‎

‎ 1978 disque Etats Uis, 1978, Giorno Poetry System GPS 012-013, 2 disques 33trs, 30cm, sous pochette ouvrante, conception et photographies de Les Levine.The Dial-a-Poem poets Big Ego.Avec, Helen Adam, Laurie Anderson, Robert Ashley, Jim Brodey, Otis Brown, William S. Burroughs, Jackie Curtis, Mona DaVinci, Kenward Elmslie, The Fugs, John Giorno, Philip Glass, Anthony J. Gnazzo, Ted Greenwald, Steve Hamilton, Bernard Heidsieck, Joe Johnson, Michael Lally, Denise Levertov, Robert Lowell, Meredith Monk, Eileen, Myles, Frank O'Hara, Claes Oldenburg, Joel Oppenheimer, Ron Padget, Ishmael Reed, Ed Sanders, Harris Schift, Patti Smith, Lorenzo Thomas, Steve & Gloria Tropp, Anne Waldman, Larry Wendt, Robert Wolson & Christopher Knowles. (103164) ‎

‎Scientia - n° VII-VIII - vol. 106 - Annus LXV - 1971‎

‎Scientia Malicorne sur Sarthe, 72, Pays de la Loire, France 1971 Book condition, Etat : Bon broché grand In-8 1 vol. - 184 pages‎

‎ Contents, Chapitres : Paginé 575 à 750 - A. Dumitriu : Histoire de la logique (1ere partie) - P. Pirlot : Relation organe-fonction et système nerveux central - S. d'Agostino : Hertz e Helmholtz sulle onde elettromagnetische - J.M. Oppenheimer : Aristotle as a Biologist - A. de Luca e S. Termini : Algorithmic aspects in complex systems analysis - I. Bolletti-Censi : Telesio - Giordano Bruno - Campanella - Reports - Books reviews a word handwritten at ink on the front-wrapper, else near fine copy, the paper is lightly browning‎

‎Arts (lettres, spectacles) n°698- Du 26 novembre au 2 décembre 1958‎

‎Rédaction Administration. 1958. In-Plano. En feuillets. Etat d'usage, Couv. défraîchie, Dos abîmé, Papier jauni. 17 pages. Rousseurs, pliures et déchirures. Quelques illustrations en noir et blanc. Texte sur plusieurs colonnes. Salissures.. . . . Classification Dewey : 70.1-Journaux‎

‎"Sommaire: Un Fémina sans audace- La science: est elle trop grande pour l'homme par Robert Oppenheimer- On nous cache des milliers de chefs-d'oeuvre- la politique de l'Etat est incohérente- le Musée imaginaire est une grande réalité- Pressés dns trois salles les ""1000"" du Tout-New York ont applaudi Picasso Classification Dewey : 70.1-Journaux"‎

‎The Monuments of Italy. A Regional Encyclopedia of Art, Architecture and Archaeology from Classical to Modern Times. 6 vols‎

‎Oppenheimer, Sir Michael: The Monuments of Italy. A Regional Encyclopedia of Art, Architecture and Archaeology from Classical to Modern Times. 6 vols. London: 2002. Together 5266pp with 828 monochrome illustrations. Cloth. 28.5x22.5cms. Lists and describes over 3500 castles, cathedrals, churches, monasteries, monuments, museums, palaces, villas, etc. describing artistic contents, architectural features and historical importance - an essential reference tool.‎

‎Lists and describes over 3500 castles, cathedrals, churches, monasteries, monuments, museums, palaces, villas, etc. describing artistic contents, architectural features and historical importance - an essential reference tool. Text in English‎

‎ Ex-libris.‎

‎Arthur u Ilse Oppenheimer (propriétaire), Ex-libris. Ex-libris (97*102mm). [284-4] ‎

‎Angoisse et complexe de castration.‎

‎ P., PUF, 1991, in 8° broché, 160 pages. ‎

‎De la Collection "Monographies de la revue française de psychanalyse". Textes de : Colette Chiland - Jean Cournut-Janin - Henz Kohut - Julia Kristeva - Bianca Lechevalier - Annick Le Guen - John Leuba - Agnès Oppenheimer - Roger Perron. ...................... Photos sur demande ..........................‎

‎La Science et le bon sens. ‎

‎Paris Gallimard 1955 Un volume in-12 broché, couverture plastifiée, 195 pages. Bon état. ‎

‎ La librairie est ouverte du mardi au samedi de 9h30 à 12h30 et de 13h30 à 19h00. Commandes par courriel ou téléphone. Envoi rapide, emballage soigné. ‎

‎L’esprit libéral‎

‎ 1957 Gallimard, 1957, in-12, 228pp.‎

‎etat parfait Ray A4* ‎

‎Kohut et la psychologie du self‎

‎PUF.1996.Bibliothèque de psychanalyse.In-8 br.couv.rempliée.301 p.avec Bibliographie.TBE‎

‎La Science et le Bon Sens. (Science and the Common Understanding)‎

‎1955, NRF, Gallimard. Traduit par A. Colnat. In-12 Br. 194 p. avec Note et Appendice. + Table. BE.‎

‎Guérir de ses angoisses avec la thérapie par téléphone‎

‎Odile Jacob (3/2023)‎

‎LIVRE A L’ETAT DE NEUF. EXPEDIE SOUS 3 JOURS OUVRES. NUMERO DE SUIVI COMMUNIQUE AVANT ENVOI, EMBALLAGE RENFORCE. EAN:9782415004484‎

‎Mountains of Fire‎

‎Hodder & Stoughton (8/2023)‎

‎LIVRE A L’ETAT DE NEUF. EXPEDIE SOUS 3 JOURS OUVRES. NUMERO DE SUIVI COMMUNIQUE AVANT ENVOI, EMBALLAGE RENFORCE. EAN:9781529351095‎

‎Colloques de Rheinfelden.‎

‎Calmann-Lévy 1960 In-8 broché 21,2 cm sur 14. 328 pages. Pages écornées et papier bruni.‎

‎ Bon état d’occasion ‎