Hans boehringer (Oltre 1000 risultati)

Condizione: Good. Good condition. A copy that has been read but remains intact. May contain markings such as bookplates, stamps, limited notes and highlighting, or a few light stains.

Paperback. Condizione: Good. No Jacket. Pages can have notes/highlighting. Spine may show signs of wear. ~ ThriftBooks: Read More, Spend Less.

Soft cover. Condizione: Very Good. No Jacket. 1st Edition. tan cover, saddle stapled with red lettering for the title and subtitle, black artwork consisting of 2 sets of double lines and cross the 2 circles over in and overlapping and surrounding for another circle, additional subtitle: The Consultation on Common Texts.…

Taschenbuch. Condizione: 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.…

Taschenbuch. Condizione: Gut. 50 Seiten; Das Taschenbuch stammt aus einer Bibliotheksauflösung. Instituts-Stempel. Sprache: Deutsch Gewicht in Gramm: 100.

Taschenbuch. Condizione: Gut. 50 Seiten, Das Buch ist ordentlich erhalten und kann altersbedingte Gebrauchsspuren aufweisen. Sprache: Deutsch Gewicht in Gramm: 150.

Hardcover. Condizione: Wie neu. XXIII, 444 S. : Ill. Like new. Shrink wrapped. Sprache: Englisch Gewicht in Gramm: 915.

Condizione: New. This is a Brand-new US Edition. This Item may be shipped from US or any other country as we have multiple locations worldwide.

Condizione: Brand New. New. US edition. Expediting shipping for all USA and Europe orders excluding PO Box. Excellent Customer Service.

Condizione: New. pp. xxiv + 446 1st Edition.

Condizione: New. pp. xxiv + 446.

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.

Original-Broschur, mit 1 ausfaltb. Karte, 91 Seiten, 15,5 x 23 cm, gut erhalten.

gr. 8° - 496 S. illustr. OPpbd., 2 CD-Roms (ungeöffnet), sehr gutes, frisches Exemplar, ohne Einträge. Die angegebenen Versandkosten können von den tatsächlichen Versandkosten (z.B. aufgrund höheren Gewichts) abweichen. The stated shipping costs may differ from the actual shipping costs (e.g. due to higher weight). Sprache: Deutsch 1420 gr.…

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.

Condizione: As New. Unread book in perfect condition.

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 ].

No Binding. Condizione: Good. First Edition. Original Printed patent disbound About 27cm by 18 cm some wear and tear due to the disbinding.

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.…

Condizione: New.

Condizione: New.

Condizione: New. In English.

Condizione: New.

Condizione: New. pp. 472.

Buch. Condizione: 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. Condizione: 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. Condizione: 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.…

Condizione: 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.…

Paperback. Condizione: New.

Condizione: New. In English.