Interstellar medium galaxies (25 Ergebnisse)

Softcover. Zustand: Gut. 556 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. K00857 792307607 Sprache: Englisch Gewicht in Gramm: 1350.

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Gr.-8°, original hardcover. 1. ed. With numerous images, XIX, 393 p. Stamp on preliminary page and title, otherwise very fine copy. Sprache: Englisch Gewicht in Gramm: 0.

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Taschenbuch. Zustand: Neu. Neuware - This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.…

Zustand: New. Invited Talks presented at the Second Teton Conference, held at Grand Teton National Park, Wyoming, USA, July 3-7, 1989 Editor(s): Thronson, Harley A., Jr; Shull, J. Michael. Series: Astrophysics and Space Science Library. Num Pages: 568 pages, 190 black & white illustrations, biography. BIC Classification: PGM. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 235 x 155 x 29. Weight in Grams: 1040. . 1990. Softcover reprint of the original 1st ed. 1990. Paperback. . . . . Books ship from the US and Ireland. …

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Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book contains the proceedings of the sixth Eurographics Workshop on Vir tual Environments. The event took place from June 1 to June 2, 2000, in Am sterdam. We hope that readers will find these proceedings to be valuable, not only for virtual environment researchers, but also for practitioners developing or using virtual environment applications. We are glad to report that visibility of the workshop continues to expand and that virtual environment researchers and practitioners from allover the world are submitting papers. This year, 40 papers and case studies were submitted of which 20 were accepted. In addition, we are glad to see that the focus of the workshop is also expanding. We accepted 6 research papers on evaluation of virtual environments and there was a broad sampling of other topics. We would like to thank all those involved in organizing the symposium. In particular, thanks go to Mieke Brune who was in charge of the local organization. In addition, we want to thank the international program committee for their excellent, yet laborious, job in reviewing all submitted papers. The quality of the workshop is a reflection of the quality of the submitted papers and the quality of the reviewing process.…

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Couverture souple. Zustand: bon. R260270042: 1990. In-8. Broché. Bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 556 pages. . . . Classification Dewey : 420-Langue anglaise. Anglo-saxon.

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Zustand: Used. pp. xx + 666 Illus.

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Zustand: New. A collection of seven reviews covering the following constituents of the interstellar medium: dust, molecular gas, neutral atomic hydrogen, ionized hydrogen, and hot gas, and covering the abundances of heavy elements in the interstellar medium and the role of star formation. It discusses the properties of constituents of the interstellar medium. Editor(s): Hulst, J.M. van der. Series: Astrophysics and Space Science Library. Num Pages: 222 pages, biography. BIC Classification: PGM. Category: (G) General (US: Trade). Dimension: 235 x 155 x 12. Weight in Grams: 710. . 2001. Softcover reprint of the original 1st ed. 1997. Paperback. . . . . Books ship from the US and Ireland.…

Zustand: New. Presenting a collection of reviews covering the following constituents of the interstellar medium: dust, molecular gas, neutral atomic hydrogen, ionized hydrogen, and hot gas, and covering the abundances of heavy elements in the interstellar medium and the role of star formation, this title is useful for professional scientists in this field. Editor(s): Hulst, J.M. van der. Series: Astrophysics and Space Science Library. Num Pages: 222 pages, biography. BIC Classification: PGM. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 234 x 156 x 14. Weight in Grams: 498. . 1997. Hardback. . . . . Books ship from the US and Ireland.…

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - It has been more than five decades ago that Henk van de Hulst predicted the observability of the 21-cm line of neutral hydrogen (HI ). Since then use of the 21-cm line has greatly improved our knowledge in many fields and has been used for galactic structure studies, studies of the interstellar medium (ISM) in the Milky Way and other galaxies, studies of the mass distribution of the Milky Way and other galaxies, studies of spiral struc ture, studies of high velocity gas in the Milky Way and other galaxies, for measuring distances using the Tully-Fisher relation etc. Regarding studies of the ISM, there have been a number of instrumen tal developments over the past decade: large CCD's became available on optical telescopes, radio synthesis offered sensitive imaging capabilities, not only in the classical 21-cm HI line but also in the mm-transitions of CO and other molecules, and X-ray imaging capabilities became available to measure the hot component of the ISM. These developments meant that Milky Way was no longer the exclusive playground for ISM studies and that by reaching out to other galaxies astronomy had gained the advantage of having an 'outside' view, though at the expense of giving up some linear resolution. Studies of the ISM in other galaxies are intimately connected to studies of the ISM in the Milky Way.…

Zustand: Sehr gut. Zustand: Sehr gut | Seiten: 688 | Sprache: Englisch | Produktart: Bücher | The¿4thCologne-Bonn-ZermattSymposium:TheDenseInterstellarMedium in Galaxies¿ took place in Zermatt, Switzerland, from September 22nd to 26th, 2003. This symposium continued the series of conferences on the dense interstellar medium which has been organized every 5 years since 1988 by the I. Physikalisches Institut der Unversit¿ at ¿ zuKoln. ¿ Re?ecting the by now well established and fruitful collaboration between the MPI ffur ¿ ¿ Radioastronomie, the Radioastronomisches Institut der Universit¿ at ¿ Bonn and the I. Physikal- ches Institut der Universit¿ at ¿ zu Koln ¿ in the context of the Sonderforschun- bereich 494 ¿The Evolution of Interstellar Matter: THz-Spectroscopy in the Laboratory and in Space¿, the symposium is now organized jointly by these three institutes. The conference covered a wide range of topics: starting at the largest scales and earliest times in the history of the Universe, it focussed next on galaxy evolution and their structure and dynamics. New and very exciting results on the black hole in the center of the Milky Way and the violent ISM in its immediate vicinity were presented. It continued on the cosmic cycle of star formation and evolution, and reached down to the microphysical p- cesses determining the physical and chemical conditions of the interstellar matter as the important agent for this cosmic cycle.…

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Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The 4thCologne-Bonn-ZermattSymposium:TheDenseInterstellarMedium in Galaxies took place in Zermatt, Switzerland, from September 22nd to 26th, 2003. This symposium continued the series of conferences on the dense interstellar medium which has been organized every 5 years since 1988 by the I. Physikalisches Institut der Unversit at zuKoln. Re ecting the by now well established and fruitful collaboration between the MPI ffur Radioastronomie, the Radioastronomisches Institut der Universit at Bonn and the I. Physikal- ches Institut der Universit at zu Koln in the context of the Sonderforschun- bereich 494 The Evolution of Interstellar Matter: THz-Spectroscopy in the Laboratory and in Space , the symposium is now organized jointly by these three institutes. The conference covered a wide range of topics: starting at the largest scales and earliest times in the history of the Universe, it focussed next on galaxy evolution and their structure and dynamics. New and very exciting results on the black hole in the center of the Milky Way and the violent ISM in its immediate vicinity were presented. It continued on the cosmic cycle of star formation and evolution, and reached down to the microphysical p- cesses determining the physical and chemical conditions of the interstellar matter as the important agent for this cosmic cycle.…

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - It has been more than five decades ago that Henk van de Hulst predicted the observability of the 21-cm line of neutral hydrogen (HI ). Since then use of the 21-cm line has greatly improved our knowledge in many fields and has been used for galactic structure studies, studies of the interstellar medium (ISM) in the Milky Way and other galaxies, studies of the mass distribution of the Milky Way and other galaxies, studies of spiral struc ture, studies of high velocity gas in the Milky Way and other galaxies, for measuring distances using the Tully-Fisher relation etc. Regarding studies of the ISM, there have been a number of instrumen tal developments over the past decade: large CCD's became available on optical telescopes, radio synthesis offered sensitive imaging capabilities, not only in the classical 21-cm HI line but also in the mm-transitions of CO and other molecules, and X-ray imaging capabilities became available to measure the hot component of the ISM. These developments meant that Milky Way was no longer the exclusive playground for ISM studies and that by reaching out to other galaxies astronomy had gained the advantage of having an 'outside' view, though at the expense of giving up some linear resolution. Studies of the ISM in other galaxies are intimately connected to studies of the ISM in the Milky Way.…