Stalio r (73 resultados)

Hardcover. Condición: Fair. The item might be beaten up but readable. May contain markings or highlighting, as well as stains, bent corners, or any other major defect, but the text is not obscured in any way. Stalio, Ivan (ilustrador).

Hardcover. Condición: Very Good. Shipped within 24 hours from our UK warehouse. Clean, undamaged book with no damage to pages and minimal wear to the cover. Spine still tight, in very good condition. Remember if you are not happy, you are covered by our 100% money back guarantee. Simone Boni; Lorenzo Cecchi; Ivan Stalio (ilustrador). …

Hardcover. Condición: Very Good. No Jacket. May have limited writing in cover pages. Pages are unmarked. ~ ThriftBooks: Read More, Spend Less. Stalio, Ivan (ilustrador).

Hardcover. Condición: Good. No Jacket. Pages can have notes/highlighting. Spine may show signs of wear. ~ ThriftBooks: Read More, Spend Less. Stalio, Ivan (ilustrador).

Hardcover. Condición: Very Good. Threatened Planet (Discovery S.) This book is in very good condition and will be shipped within 24 hours of ordering. The cover may have some limited signs of wear but the pages are clean, intact and the spine remains undamaged. This book has clearly been well maintained and looked after thus far. Money back guarantee if you are not satisfied. See all our books here, order more than 1 book and get discounted shipping. . Simone Boni; Lorenzo Cecchi; Ivan Stalio (ilustrador).…

Condición: Very Good. Bon état. 1x21x14cm. 1996. Relié. Very Good.

8°, original Hardcover. 1. ed. Numerous images, XXII, 570 p. English Edition. Cover slightly tanned, three stamps, otherwise very fine copy. Sprache: Englisch Gewicht in Gramm: 0.

Gr.-8°, Original hardcover. 1. ed. With numerous fig., XXI, 566 p. Stamp on title, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.

Gr.-8°, original hardcover. 1. ed. Numerous fig.,XII, 365 p. Shelfmark on spine, stamp on title, otherwise very fine copy. Sprache: Englisch Gewicht in Gramm: 0.

Gr.-8°, original hardcover. 1. ed. XII, 336 p. Stamp on preliminary page and title, otherwise very fine copy. Sprache: Englisch Gewicht in Gramm: 0.

Hard Cover. Condición: Good. No Jacket. First Edition. From an academic library with the usual stamps and labels. This item is heavy and will attract postal surcharges. Binding is card boards. Boards sunned to edges and spine. A00005884.

Hard Cover. Condición: Good. No Jacket. First Edition. From an academic library with the usual stamps and labels. This item is heavy and will attract postal surcharges. Binding is card boards with canvas spine. Boards sunned to edges. A00005884.

hardcover. Condición: new. Stalio, Ivan (ilustrador).

hardcover. Condición: New. In shrink wrap. Looks like an interesting title. Stalio, Ivan (ilustrador).

Condición: Good. Former library copy. Pages intact with minimal writing/highlighting. The binding may be loose and creased. Dust jackets/supplements are not included. Includes library markings. Stock photo provided. Product includes identifying sticker. Better World Books: Buy Books. Do Good.

Condición: New.

Condición: New.

Taschenbuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - Stellar mass loss is an essential part of the cycling of material from the interstellar medium into stars and back, and must be understood if we are to model processes on galactic to cosmological scales. The study of stellar winds and the effects of stellar mass loss has reached a particularly exciting stage where observational capabilities are increasingly able to provide interesting constraints on models and theories. Recent resu1ts from theoretical and observational work for both hot and cool stars with substantial winds have led to the suggestion that a combination of pulsation with other mechanisms makes for particularly efficient mass loss from stars. This provided the original motivation for the organization of this workshop. The conference was organized along relatively conventional lines according to the types of objects being scrutinized. However the true unity of the proceedings comes from the interplay of the mechanisms involved. For example, for the cool, luminous Mira variables, pulsation leads to shock waves that extend the atmosphere, enhancing dust formation; radiation pressure on dust drives the wind, cooling the atmosphere and in some cases suppressing the shocks. Similarly for the Be stars, both pulsation (in this case, non-radial) and radiation pressure (due to UV resonance lines) are expected to be important, and this expectation is at least qualitatively borne out by the observations.…

Buch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - Stellar mass loss is an essential part of the cycling of material from the interstellar medium into stars and back, and must be understood if we are to model processes on galactic to cosmological scales. The study of stellar winds and the effects of stellar mass loss has reached a particularly exciting stage where observational capabilities are increasingly able to provide interesting constraints on models and theories. Recent resu1ts from theoretical and observational work for both hot and cool stars with substantial winds have led to the suggestion that a combination of pulsation with other mechanisms makes for particularly efficient mass loss from stars. This provided the original motivation for the organization of this workshop. The conference was organized along relatively conventional lines according to the types of objects being scrutinized. However the true unity of the proceedings comes from the interplay of the mechanisms involved. For example, for the cool, luminous Mira variables, pulsation leads to shock waves that extend the atmosphere, enhancing dust formation; radiation pressure on dust drives the wind, cooling the atmosphere and in some cases suppressing the shocks. Similarly for the Be stars, both pulsation (in this case, non-radial) and radiation pressure (due to UV resonance lines) are expected to be important, and this expectation is at least qualitatively borne out by the observations.…

Condición: New.

Condición: New.

Condición: New.

Condición: As New. Unread book in perfect condition.

Condición: New. pp. 352.

Condición: New.

Condición: As New. Unread book in perfect condition.

Condición: As New. Unread book in perfect condition.

Condición: As New. Unread book in perfect condition.

Gebunden. Condición: New. Proceedings of IAU Colloquium No. 59 held in Miramare, Trieste, Italy, September 15-19, 1980 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 Physic.

Paperback. Condición: Brand New. 352 pages. 9.25x6.10x0.80 inches. In Stock.