Language: German
Published by Düsseldorf : Patmos-Verlag, 1975
ISBN 10: 3491774055 ISBN 13: 9783491774056
Seller: books4less (Versandantiquariat Petra Gros GmbH & Co. KG), Welling, Germany
Taschenbuch. Condition: Gut. 169 S. Das hier angebotene Buch stammt aus einer teilaufgelösten Bibliothek und kann die entsprechenden Kennzeichnungen aufweisen (Rückenschild, Instituts-Stempel.); der Buchzustand ist ansonsten ordentlich und dem Alter entsprechend gut. Sprache: Deutsch Gewicht in Gramm: 220.
Language: German
Published by Seelsorge-Verlag, 1961
Seller: books4less (Versandantiquariat Petra Gros GmbH & Co. KG), Welling, Germany
Taschenbuch. Condition: Gut. 50 Seiten; Das Taschenbuch stammt aus einer Bibliotheksauflösung. Instituts-Stempel. Sprache: Deutsch Gewicht in Gramm: 100.
Language: German
Published by Seelsorge Verlag 1961,., 1961
Seller: books4less (Versandantiquariat Petra Gros GmbH & Co. KG), Welling, Germany
Taschenbuch, Condition: Gut. 50 Seiten, Das Buch ist ordentlich erhalten und kann altersbedingte Gebrauchsspuren aufweisen. Sprache: Deutsch Gewicht in Gramm: 150.
Seller: Antiquariat Thomas Haker GmbH & Co. KG, Berlin, Germany
Association Member: GIAQ
Hardcover. Condition: Wie neu. XXIII, 444 S. : Ill. Like new. Shrink wrapped. Sprache: Englisch Gewicht in Gramm: 915.
Condition: Brand New. New. US edition. Expediting shipping for all USA and Europe orders excluding PO Box. Excellent Customer Service.
Condition: New. Brand New Original US Edition. Customer service! Satisfaction Guaranteed.
Seller: Books Puddle, New York, NY, U.S.A.
Condition: New. pp. xxiv + 446 1st Edition.
Seller: Biblios, Frankfurt am main, HESSE, Germany
Condition: New. pp. xxiv + 446.
Published by New York Academy of Sciences, NY, 1995
Seller: Neil Shillington: Bookdealer/Booksearch, Hobe sound, FL, U.S.A.
large paperbac. 728 pages VG++ Annals of the NY Academy of Science Volume 759, very scarce.
Language: German
Published by Hoheneck-Verlag, Hamm,, 1965
Seller: Clerc Fremin, Steingaden, Germany
Softcover, Heft. 20 Seiten Die Jahresangabe ist ungefähr. Zustand: keine Beschädigungen, eine Eintragung auf letzter Seite. Rücken, Ecken, Kanten gut. Sprache: Deutsch Gewicht in Gramm: 200.
Language: English
Published by New York Academy of Sciences, 1995
ISBN 10: 0897669428 ISBN 13: 9780897669429
Seller: Antiquariat Dr. Rainer Minx, Bücherstadt, Zeuthen, Germany
8°, Broschiert. Einige s/w Abb., 728 S.; Text in engl. Spr., Einb. und Kanten gering bestoßen, ansonsten kaum Gebrauchsspuren vorhanden, gutes Exemplar Sprache: Englisch Gewicht in Gramm: 1500.
Language: English
Published by Walther König / Schaulager Basel, 2004
ISBN 10: 3952296708 ISBN 13: 9783952296707
Seller: Antiquariat UEBUE, Zürich, Switzerland
Softcover. Condition: Sehr gut. Z : 194 Seiten, 13 x 21 cm, illustriert - Das Buch vereinigt die Beiträge des Symposiums, das am 4. und 5. Juli 2003 anlässlich der Ausstellung «Roth Zeit. Eine Dieter Roth Retrospektive» im Schaulager Basel stattgefunden hat. Vorgestellt und diskutiert werden in den Beiträgen und Aufsätzen Werkprozesse, die Wahl des Materials, die Rolle des Abfalls und das Atelier als Ausstellung sowie das Verhältnis von Schrift und Bild und der Zusammenhang von Kunst und Leben im Schaffen und Denken Dieter Roths.
Published by Zürich Leemann & Co, 1935
Seller: Libretto Antiquariat & mundart.ch, Langnau i.E., BE, Switzerland
Original-Broschur, mit 1 ausfaltb. Karte, 91 Seiten, 15,5 x 23 cm, gut erhalten.
Condition: As New. Unread book in perfect condition.
Language: English
Published by Max-Planck-Institut für extraterrestrische Physik, Garching, 1993
Seller: Antiquariat Silvanus - Inhaber Johannes Schaefer, Ahrbrück, Germany
177 S. mit Abbildungen, Als Manuskript gedruckt. Printed as a script. Sprache: Englisch Gewicht in Gramm: 550 4°, Original-Karton (Softcover), Deckel mit kleinem Namensstempel, insgesamt gutes und innen sauberes Exemplar,
Language: German
Published by Akademie der Diözese Rottenburg,, 1967
Seller: Clerc Fremin, Steingaden, Germany
Softcover. 65 Seiten Nur Nr. 82. Zustand: Keine Beschädigungen, mit einer Namenseintragung im Vorsatz. Rücken, Ecken, Kanten gut. Mit einem zusätzlichen Folieneinband (keine Klebefolie). Sprache: Deutsch Gewicht in Gramm: 150.
Published by Stuttgart, Wegra, 1979., 1979
Seller: Antiquariat Hohmann, Schemmerhofen, Germany
First Edition
212 S., zahlr. Abb., gr.okt., ill. Pp., SchU., (2) mehrf. gef. Ktn.- [ Landeskunde Geschichte DE707 Zeit1229 -Zeit1979 J| 1979 N| Wilfried Setzler N| Dieter Böhringer N| Herbert Bühler N| Rainer Häußler N| Lothar Reinhard N| Hans Georg Hofacker | 89697 ].
Seller: Ria Christie Collections, Uxbridge, United Kingdom
£ 50.80
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Published by Freiburg i. Br. : Seelsorge-Verl., 1961
Seller: Roland Antiquariat UG haftungsbeschränkt, Weinheim, Germany
Taschenbuch. o.A. 50 S. Leichte Lager- und Gebrauchsspuren. Ausgeschiedenes Bibliotheksexemplar mit den üblichen Kennzeichnungen, Einband leicht verschmutzt. Ansonsten innen wie außen ein sehr gutes Exemplar. Die Leseseiten sind sauber und ohne Anstreichungen oder Knicke. Sprache: Deutsch Gewicht in Gramm: 200.
Condition: New.
Seller: Books Puddle, New York, NY, U.S.A.
Condition: New. pp. 472.
Language: English
Published by Springer Berlin Heidelberg, 2010
ISBN 10: 3642092578 ISBN 13: 9783642092572
Seller: AHA-BUCH GmbH, Einbeck, Germany
Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - The Universe would be a dull and dark place if the gaseous baryons did not cool, collapse, and form stars and galaxies. However, if this gas is allowed to cool unimpeded at the rate predicted from known atomic physics, in the context of a well-established cosmological model, the gaseous matter would form stars and galaxies with a high e ciency, so that far more than the observed fraction of about 10-15% of the baryonic matter would be found in luminous stellar systems. Therefore,cooling must be damped or regulatedby heating processes, and observations show that this 'feedback' is a widespread astrophysical phenomenon. The place where this cooling and feedback manifests itself most dram- ically is in the inner regions of the most massive Dark Matter halos found in our Universe, in the cores of galaxy clusters. The e ect of cosmic co- ing in these objects was recognized in the mid-1970s, and the term 'cooling ow' was introduced by Andy Fabian and colleagues at Cambridge as a p- sible explanation of the physical processes obtained in the central regions of clusters. The name refers to the fact that gas cooling in the inner regions is associated with a loss of central pressure, causing an in ow of hot gas from larger radii.
Taschenbuch. Condition: Neu. Heating versus Cooling in Galaxies and Clusters of Galaxies | Proceedings of the MPA/ESO/MPE/USM Joint Astronomy Conference held in Garching, Germany, 6-11 August 2006 | Hans Böhringer (u. a.) | Taschenbuch | xxiii | Englisch | 2010 | Springer | EAN 9783642092572 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.
Condition: Sehr gut. Zustand: Sehr gut | Seiten: 472 | Sprache: Englisch | Produktart: Bücher | The Universe would be a dull and dark place if the gaseous baryons did not cool, collapse, and form stars and galaxies. However, if this gas is allowed to cool unimpeded at the rate predicted from known atomic physics, in the context of a well-established cosmological model, the gaseous matter would form stars and galaxies with a high e?ciency, so that far more than the observed fraction of about 10¿15% of the baryonic matter would be found in luminous stellar systems. Therefore,cooling must be damped or regulatedby heating processes, and observations show that this ¿feedback¿ is a widespread astrophysical phenomenon. The place where this cooling and feedback manifests itself most dram- ically is in the inner regions of the most massive Dark Matter halos found in our Universe, in the cores of galaxy clusters. The e?ect of cosmic co- ing in these objects was recognized in the mid-1970s, and the term ¿cooling ?ow¿ was introduced by Andy Fabian and colleagues at Cambridge as a p- sible explanation of the physical processes obtained in the central regions of clusters. The name refers to the fact that gas cooling in the inner regions is associated with a loss of central pressure, causing an in?ow of hot gas from larger radii.
Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - The Universe would be a dull and dark place if the gaseous baryons did not cool, collapse, and form stars and galaxies. However, if this gas is allowed to cool unimpeded at the rate predicted from known atomic physics, in the context of a well-established cosmological model, the gaseous matter would form stars and galaxies with a high e ciency, so that far more than the observed fraction of about 10-15% of the baryonic matter would be found in luminous stellar systems. Therefore,cooling must be damped or regulatedby heating processes, and observations show that this 'feedback' is a widespread astrophysical phenomenon. The place where this cooling and feedback manifests itself most dram- ically is in the inner regions of the most massive Dark Matter halos found in our Universe, in the cores of galaxy clusters. The e ect of cosmic co- ing in these objects was recognized in the mid-1970s, and the term 'cooling ow' was introduced by Andy Fabian and colleagues at Cambridge as a p- sible explanation of the physical processes obtained in the central regions of clusters. The name refers to the fact that gas cooling in the inner regions is associated with a loss of central pressure, causing an in ow of hot gas from larger radii.
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Paperback. Condition: New.
Seller: GreatBookPricesUK, Woodford Green, United Kingdom
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