Marshal wrubel (23 resultados)

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Paperback or Softback. Condición: New. A Primer of Programming for Digital Computers: McGraw-Hill Series in Information Processing and Computers. Book.

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Condición: As New. Unread book in perfect condition.

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Softcover. Originalbroschur gr. 8° 419-423 SS. m. 2 Figuren. ausgeschiedenes Bibliotheksexemplar. etwas gebräunt. sehr guter Zustand. Reprinted from Stellar Evolution". Reprint of the Goethe Link Observatory, Indiana University, No. 38. in englischer Sprache (in english).

Originalbroschur gr. 8°. 107-116 Seiten. m. 5 Figuren. ausgeschiedenes Bibliotheksexemplar. etwas berieben. angerändert, gebräunt. sehr guter Zustand. Reptrinted from Vistas in Astronomy", Vol. III. Reprint of the Goethe Link Observatory, Indiana University, No. 22. in englischer Sprache (in english).…

Softcover. Originalbroschur gr. 8° 8° nn. Seiten. ausgeschiedenes Bibliotheksexemplar. m.leichten Gebrauchsspuren. sehr guter Zustand. Reprinted from The Review" 1961. Reprint of the Goethe Link Observatory, Indiana University, No. 30. in englischer Sprache (in english).

Condición: New.

Condición: New.

Condición: New. In English.

Taschenbuch. Condición: Neu. Astrophysik II: Sternaufbau / Astrophysics II: Stellar Structure | Marshal H. Wrubel (u. a.) | Taschenbuch | Handbuch der Physik Encyclopedia of Physics | viii | Englisch | 2012 | Springer | EAN 9783642459108 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu. …

Condición: New. pp. 840.

Paperback. Condición: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

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Leatherbound. Condición: NEW. BOOKS ARE EXEMPT FROM IMPORT DUTIES AND TARIFFS; NO EXTRA CHARGES APPLY. Leatherbound edition. Condition: New. Leather Binding on Spine and Corners with Golden leaf printing on spine. Bound in genuine leather with Satin ribbon page markers and Spine with raised gilt bands. Pages: 258. A perfect gift for your loved ones. Reprinted from 1959 edition. NO changes have been made to the original text. This is NOT a retyped or an ocr'd reprint. Illustrations, Index, if any, are included in black and white. Each page is checked manually before printing. As this print on demand book is reprinted from a very old book, there could be some missing or flawed pages, but we always try to make the book as complete as possible. Fold-outs, if any, are not part of the book. If the original book was published in multiple volumes then this reprint is of only one volume, not the whole set. IF YOU WISH TO ORDER PARTICULAR VOLUME OR ALL THE VOLUMES YOU CAN CONTACT US. Resized as per current standards. Sewing binding for longer life, where the book block is actually sewn (smythe sewn/section sewn) with thread before binding which results in a more durable type of binding. Language: English Pages: 258.…

Soft cover. Condición: Very Good. 1st Edition. VERY GOOD; FIRST EDITION; various papers presented at Indiana University in 1954 by leading astronomers in stellar atmospheres; some edge browning and scrapes to the cover but otherwise in very nice condition; the pages inside are clean and unmarked and the binding is solid; 8vo - over 7¾" - 9¾" tall Size: 8vo - over 7¾" - 9¾" tall.…

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Taschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Sects. 12, 13. 89 sequence and that subgiant and fainter stars in globular clusters have ultraviolet excesses. When dealing with stars whose physical properties are imperfectly under stood, such as in globular cluster stars, we cannot rely too heavily on the empiri cal calibration by the kinds of stars used to define Fig. 5, to determine their true, unreddened U-B, B-V curve. But if by a combination of arguments, principally the reddening in the region of the stars we do known about, we can assign a fairly probable unreddened U-B, B-V curve to a group of stars about which we know little, the argument may be turned around. In this case some information may be gained about the energy envelope of the stars by examining the differences between the normal two-color index curves for the unknown group of stars compared to the known. In general there seem to be two possible causes for different stars defining different normal sequences in the U-B, B-V plane. One, the relative energy distribution in the continuum in the U, B and V photometry bands are different. An example of this is the effect of the Balmer depression in supergiants. This, of course, requires deviation from black body radiation curves for one or both groups of stars. This cause seems to be the dominant effect for very blue, hot stars where the depression of the continuum by absorption lines is at a minimum. 840 pp. Englisch.…

Taschenbuch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -Sects. 12, 13. 89 sequence and that subgiant and fainter stars in globular clusters have ultraviolet excesses. When dealing with stars whose physical properties are imperfectly under stood, such as in globular cluster stars, we cannot rely too heavily on the empiri cal calibration by the kinds of stars used to define Fig. 5, to determine their true, unreddened U-B, B-V curve. But if by a combination of arguments, principally the reddening in the region of the stars we do known about, we can assign a fairly probable unreddened U-B, B-V curve to a group of stars about which we know little, the argument may be turned around. In this case some information may be gained about the energy envelope of the stars by examining the differences between the normal two-color index curves for the unknown group of stars compared to the known. In general there seem to be two possible causes for different stars defining different normal sequences in the U-B, B-V plane. One, the relative energy distribution in the continuum in the U, B and V photometry bands are different. An example of this is the effect of the Balmer depression in supergiants. This, of course, requires deviation from black body radiation curves for one or both groups of stars. This cause seems to be the dominant effect for very blue, hot stars where the depression of the continuum by absorption lines is at a minimum.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 840 pp. Englisch.…

Condición: New. PRINT ON DEMAND pp. 840.

Condición: New. Print on Demand pp. 840 197 Figures, 67:B&W 6.69 x 9.61 in or 244 x 170 mm (Pinched Crown) Perfect Bound on White w/Gloss Lam.