Published by Dordrecht u.a., Reidel Publishing,, 1979
Language: English
First Edition
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Add to basket1. ed. With various illustr., VII, 280 p. Stamp on preliminary page and title, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0 Gr.-8°, Original Cloth Binding.
Published by Springer Netherlands, 1979
ISBN 10: 9027710015 ISBN 13: 9789027710017
Language: English
Seller: Better World Books Ltd, Dunfermline, United Kingdom
US$ 63.65
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Add to basketCondition: Good. 1979th Edition. Ships from the UK. Former library book; may include library markings. Used book that is in clean, average condition without any missing pages.
Published by Dordrecht et al., D. Reidel,, 1979
Language: English
First Edition
US$ 45.65
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Add to basketGr.-8°, original clothbound. 1. ed. VII, 280 p. English Edition. Shelfmark, stamp on title and preliminary page, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.
First Edition
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Add to basketHard Cover. Condition: Good. No Jacket. First Edition. From an academic library with the usual stamps and labels. This item is heavy and will attract postal surcharges. Boards thumbed. A00005977.
Seller: GreatBookPrices, Columbia, MD, U.S.A.
Condition: New.
Seller: Lucky's Textbooks, Dallas, TX, U.S.A.
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Seller: GreatBookPrices, Columbia, MD, U.S.A.
Condition: New.
Seller: Lucky's Textbooks, Dallas, TX, U.S.A.
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Seller: Die Buchgeister, Ludwigsburg, BW, Germany
US$ 4.19
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Add to basketTaschenbuch. Condition: Gut. Aufl. 1979, Volume 77 * Einband: leicht fleckig, leicht nachgedunkelt, Ecken angestoßen * Seiten: leichte Lesespuren * Datumsstempel.
Seller: GreatBookPrices, Columbia, MD, U.S.A.
Condition: As New. Unread book in perfect condition.
Seller: GreatBookPrices, Columbia, MD, U.S.A.
Condition: As New. Unread book in perfect condition.
Seller: Ria Christie Collections, Uxbridge, United Kingdom
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Seller: Ria Christie Collections, Uxbridge, United Kingdom
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Published by Springer Netherlands, Springer Netherlands, 1979
ISBN 10: 9027710015 ISBN 13: 9789027710017
Language: English
Seller: AHA-BUCH GmbH, Einbeck, Germany
US$ 135.66
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Add to basketBuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - Eclipsing Variables - What They can Tell Us and What We can do with Them The aim of the present book will be to provide an introduction to the inter pretation of the observed light changes of eclipsing binary stars and their analysis for the elements of the respective systems. Whenever we study the properties of any celestial body - be it a planet or a star - all information we wish to gain can reach us through two different channels: their gravitational attraction, and their light. Gravitational interaction between our Earth and its celestial neighbours is, however, measurable only at distances of the order of the dimensions of our solar system; and the only means of communication with the realm of the stars are their nimble-footed photons reaching us - with appropriate time-lag - across the intervening gaps of space. As long as a star is single and emits constant light, it does not constitute a very revealing source of information. A spectrometry of its light can disclose, to be sure, the temperature (colour, or ionization) of the star's semi-transparent outer layers, their chemical composition, and prevalent pressure (through Stark effect) or magnetic field (Zeeman effect), it can disclose even some information about its absolute luminosity or rate of spin. It cannot, however, tell us anything about what we should like to know most - namely, the mass or size (i.e., density) of the respective configuration; its absolute dimensions, or its internal structure.
Published by Springer Netherlands, 1979
ISBN 10: 9027710449 ISBN 13: 9789027710444
Language: English
Seller: AHA-BUCH GmbH, Einbeck, Germany
US$ 137.37
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Add to basketTaschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - Eclipsing Variables - What They can Tell Us and What We can do with Them The aim of the present book will be to provide an introduction to the inter pretation of the observed light changes of eclipsing binary stars and their analysis for the elements of the respective systems. Whenever we study the properties of any celestial body - be it a planet or a star - all information we wish to gain can reach us through two different channels: their gravitational attraction, and their light. Gravitational interaction between our Earth and its celestial neighbours is, however, measurable only at distances of the order of the dimensions of our solar system; and the only means of communication with the realm of the stars are their nimble-footed photons reaching us - with appropriate time-lag - across the intervening gaps of space. As long as a star is single and emits constant light, it does not constitute a very revealing source of information. A spectrometry of its light can disclose, to be sure, the temperature (colour, or ionization) of the star's semi-transparent outer layers, their chemical composition, and prevalent pressure (through Stark effect) or magnetic field (Zeeman effect), it can disclose even some information about its absolute luminosity or rate of spin. It cannot, however, tell us anything about what we should like to know most - namely, the mass or size (i.e., density) of the respective configuration; its absolute dimensions, or its internal structure.