chiosi (34 Ergebnisse)

Zustand: acceptable. Ausreichend/Acceptable: Exemplar mit vollständigem Text und sämtlichen Abbildungen oder Karten. Schmutztitel oder Vorsatz können fehlen. Einband bzw. Schutzumschlag weisen unter Umständen starke Gebrauchsspuren auf. / Describes a book or dust jacket that has the complete text pages (including those with maps or plates) but may lack endpapers, half-title, etc. (which must be noted). Binding, dust jacket (if any), etc may also be worn.

Hard cover. Zustand: Very Good. Large 8vo 9" - 10" tall; 397 pages; D Reidel HC in original pale blue boards with titles in dark blue to spine and cover. Library ownership indications; call label spine; bookplate front pastedown and card pocket rear. Appears unread. No marks aside from library ownership. Faint sunning to board edges/spine. VG-to VG.

Zustand: Good. Most items will be dispatched the same or the next working day. A copy that has been read but remains in clean condition. All of the pages are intact and the cover is intact and the spine may show signs of wear. The book may have minor markings which are not specifically mentioned.

Zustand: New. In.

Zustand: NEW.

Hardcover. XIV-397 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. D03844 902771729X Sprache: Englisch Gewicht in Gramm: 550.

paperback. Zustand: Good. Zustand des Schutzumschlags: No Dust Jacket. Paperback in good condition. Ex-library. Light creases on spine and rear cover. Bottom of page block is grubby. Library stamps and numbers on title page, otherwise pages are clean and tight throughout. Profusely illustrated by diagrams and tables. T. Used.

Zustand: NEW.

Zustand: New. In.

Zustand: New. In.

Zustand: new.

Illustr. Pappband Hardcover. Zustand: Guter Zustand. Zustand des Schutzumschlags: Kein Schutzumschlag. First Edition. proceedings of the fourth workshop of the advanced school of astronomy of the " ettore majorana " centre for scientific culture, erice, italy, march 12 - 22, 1985; XII, 490 pages with figures; book with two owner stamps, little signs of use - good condition; 1,5 kg shipping weight;

Paperback. Zustand: Brand New. 416 pages. 9.60x6.69x0.94 inches. In Stock.

Paperback. Zustand: Brand New. 492 pages. 9.25x6.10x1.11 inches. In Stock.

Taschenbuch. Zustand: Neu. Stellar Nucleosynthesis | Proceedings of the Third Workshop of the Advanced School of Astronomy of the Ettore Majorana Centre for Scientific Culture, Erice, Italy, May 11-21, 1983 | C. Chiosi (u. a.) | Taschenbuch | Astrophysics and Space Science Library | 411 S. | Englisch | 2011 | Springer | EAN 9789400963504 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - x about a sequence of reVlew lectures, each followed by contributed talks and discussions. The opening session was devoted to reviewing the most recent results concerning the determination of chemical abundances in particularly inte resting objects providing direct evidence for stellar nucleosynthesis (like planetary nebulae, supernovae and supernova remnants). In Session 2 recent results on some relevant nuclear reaction rates have been presented. Session 3 grouped the contributions concerning the quasi-static evolution of normal stars, its relevance for the nucleosynthesis of the varlOUS elements and isotopes, and the comparison of the evolutionary models with the observations. Session 4 addressed the important questions of identifying the precursors of both Type I and Type II supernovae, and of determining the detailed composition of the ejecta by explosive nucleosynthesis associated with these events. Finally, Session 5 was devoted to a presentation of recent calculations of the evolution of hypothetical pre-galactic very massive objects (in cluding their potential role in pre-galactic nucleosynthesis), and to reviewing the progress that has been made in understanding the chemical evolution of galaxies. The discussion during and after talks was spirited and contributed signi ficantly to the succes of the workshop. We regrett for not having been able of reporting it 'in toto' in the proceedings. Nevertheless, we hope that what has been recorded may still give to the reader at least part of the excitement we have experienced during the ten days of the workshop.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Recent years have witnessed the expansion and multiplication of the observations of star formation and fragmentation accompanied by a consequent growth in the study of the underlying physical processes, the chemistry, the sites, the times, etc. Moreover, recent studies have shown that the formation of stars is likely to share many features with the formation of other self-gravitating objects. The present volume, therefore, discusses the formation of such objects in a systematic and comparative manner.

Zustand: Sehr gut. Zustand: Sehr gut | Seiten: 492 | Sprache: Englisch | Produktart: Bücher | Recent years have witnessed the expansion and multiplication of the observations of star formation and fragmentation accompanied by a consequent growth in the study of the underlying physical processes, the chemistry, the sites, the times, etc. Moreover, recent studies have shown that the formation of stars is likely to share many features with the formation of other self-gravitating objects. The present volume, therefore, discusses the formation of such objects in a systematic and comparative manner.

Zustand: New. In.

Zustand: New. In.

Zustand: New. In.

Zustand: New. In.

Taschenbuch. Zustand: Neu. Effects of Mass Loss on Stellar Evolution | IAU Colloquium no. 59 Held in Miramare, Trieste, Italy, September 15-19, 1980 | C. Chiosi (u. a.) | Taschenbuch | Astrophysics and Space Science Library | xxii | Englisch | 2011 | Springer | EAN 9789400985025 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.

Zustand: New. Proceedings of the Fourth Workshop on the Advanced School of Astronomy of the Ettore Majorana Centre for Scientific Culture, Erice, Italy, March 12-22, 1985 As it was said by one of the participants to this workshop In our attempts to understand th.

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - As it was said by one of the participants to this workshop' In our attempts to understand the spectral evolution of galaxies, we are fortunate indeed to have the ability to look back in time and observe galaxies as they were billions of years ago. Perhaos in no other discipline is it possible to gain such a direct view to hJstory. The galaxies we seek to study are remote, their light faint, and thus only recently has it become technicaJlv feasible to sample the spectra of normal luminosity galaxies at lookback times of five billion years or more' . or, perhaps. even to see galaxies in the process of their formation. or shortly afterwards. This fourth workshop organized by the 'Advanced School ot Astronomy was indeed centered on the 'Spectral Evolution of Galaxies'. on reviewing and discussing the relevant astrophysical processes and on assessing our current ability to model and understand the evolution of stellar populations. Following an opening session dealing with some outstanding questions of galaxy evolution. Session I addressed the specific problems of galaxy and star formation processes. topics of uncertainty and controversy to which IRAS observations may give novel perspectives. The properties of stellar populations in the local group of galaxies formed the basis of Session II. Session III dealt with the fundaments of the theory of spectral and photometrical evolution of stellar populations. and with recent developments in the theory of stellar structure. a necessary step to model and understand galactic evolution.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The IAU Colloquium No. 59, 'The effects of mass loss on Stellar Evolution' was held on September 15-19, 1980 at the International Centre for Theoretical Physics, Miramare, Trieste (Italy), under the auspices of the IAU Executive Co~ mittee and the Italian National Council of Research. The planning of this conference began two years ago du ring the IAU Symposium No. 83 'Mass loss and evolution of 0 type stars' (Qualicum Beach, Victoria, Canada) when we felt that mass loss and its effects on the evolution of stars was too broad a subject for being confined to 0 type stars only. Therefore we thought that a conference dealing with the general problem of mass loss across the whole HR diagram would have been of interest to all people working in the field. The main idea was that bringing together Astronomers and Astrophysicists of the widest range of interests and e~ pertize - all in some way related to the problem of mass loss from stars - would have spurred thorough discussions on the many aspects and implications of this topic. We hope this goal has been achieved. Furthermore, the most recent observational and theoreti cal developments on the problem of mass loss from early ty pe stars avoided this meeting to be a simple updating of the Qualicum Beach Symposium as far as this issue is concerned.

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The IAU Colloquium No. 59, 'The effects of mass loss on Stellar Evolution' was held on September 15-19, 1980 at the International Centre for Theoretical Physics, Miramare, Trieste (Italy), under the auspices of the IAU Executive Co~ mittee and the Italian National Council of Research. The planning of this conference began two years ago du ring the IAU Symposium No. 83 'Mass loss and evolution of 0 type stars' (Qualicum Beach, Victoria, Canada) when we felt that mass loss and its effects on the evolution of stars was too broad a subject for being confined to 0 type stars only. Therefore we thought that a conference dealing with the general problem of mass loss across the whole HR diagram would have been of interest to all people working in the field. The main idea was that bringing together Astronomers and Astrophysicists of the widest range of interests and e~ pertize - all in some way related to the problem of mass loss from stars - would have spurred thorough discussions on the many aspects and implications of this topic. We hope this goal has been achieved. Furthermore, the most recent observational and theoreti cal developments on the problem of mass loss from early ty pe stars avoided this meeting to be a simple updating of the Qualicum Beach Symposium as far as this issue is concerned.

Paperback. Zustand: Brand New. 508 pages. 9.25x6.10x1.15 inches. In Stock.

Paperback. Zustand: Brand New. 596 pages. 9.25x6.10x1.35 inches. In Stock.

Taschenbuch. Zustand: Neu. Neuware - As it was said by one of the participants to this workshop' In our attempts to understand the spectral evolution of galaxies, we are fortunate indeed to have the ability to look back in time and observe galaxies as they were billions of years ago. Perhaos in no other discipline is it possible to gain such a direct view to hJstory. The galaxies we seek to study are remote, their light faint, and thus only recently has it become technicaJlv feasible to sample the spectra of normal luminosity galaxies at lookback times of five billion years or more' . or, perhaps. even to see galaxies in the process of their formation. or shortly afterwards. This fourth workshop organized by the 'Advanced School ot Astronomy was indeed centered on the 'Spectral Evolution of Galaxies'. on reviewing and discussing the relevant astrophysical processes and on assessing our current ability to model and understand the evolution of stellar populations. Following an opening session dealing with some outstanding questions of galaxy evolution. Session I addressed the specific problems of galaxy and star formation processes. topics of uncertainty and controversy to which IRAS observations may give novel perspectives. The properties of stellar populations in the local group of galaxies formed the basis of Session II. Session III dealt with the fundaments of the theory of spectral and photometrical evolution of stellar populations. and with recent developments in the theory of stellar structure. a necessary step to model and understand galactic evolution.