Synopsis
The evolution and energy production process of stars is dependent on their masses. Stars are observed to lose mass during their evolution along the Red Giant Branch (RGB). Therefore, by the time stars reach the Red Giant Clump (RGC), they are said to have undergone enormous mass loss. This may inturn affect the evolutionary path of these stars. Using the data from the Kepler open cluster, NGC 6819, the masses of stars along the RGB and RGC were obtained using the asteroseismic parameters (such as maximum pulsational frequency and large frequency separation). The age of the RGC stars was obtained using the age - metallicity relation. The mass loss mechanisms, amount of mass lost by stars from RGB to RGC, the effect of mass loss on the distribution of stars at the Clump are discussed in detail in this book.
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About the Author
I am a teaching assistant in the Department of Physics, Faculty of Science, Mbarara University of Science and Technology (MUST) located in Mbarara, Uganda. I hold a Masters degree in Physics and a Bachelors degree in Science with Education. I enjoy doing research in Astrophysics especially in the area of stellar Astrophysics
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Mass Loss and Age of the RGC Stars in the Kepler Cluster NGC 6819
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LAP LAMBERT Academic Publishing Nov 2014, 2014
ISBN 10: 3659637149
ISBN 13: 9783659637148
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Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The evolution and energy production process of stars is dependent on their masses. Stars are observed to lose mass during their evolution along the Red Giant Branch (RGB). Therefore, by the time stars reach the Red Giant Clump (RGC), they are said to have undergone enormous mass loss. This may inturn affect the evolutionary path of these stars. Using the data from the Kepler open cluster, NGC 6819, the masses of stars along the RGB and RGC were obtained using the asteroseismic parameters (such as maximum pulsational frequency and large frequency separation). The age of the RGC stars was obtained using the age - metallicity relation. The mass loss mechanisms, amount of mass lost by stars from RGB to RGC, the effect of mass loss on the distribution of stars at the Clump are discussed in detail in this book. 96 pp. Englisch. Seller Inventory # 9783659637148
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Mass Loss and Age of the RGC Stars in the Kepler Cluster NGC 6819
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ISBN 13: 9783659637148
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Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Nsamba BenardI am a teaching assistant in the Department of Physics, Faculty of Science, Mbarara University of Science and Technology (MUST) located in Mbarara, Uganda. I hold a Masters degree in Physics and a Bachelors degree in Sci. Seller Inventory # 5170142
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Mass Loss and Age of the RGC Stars in the Kepler Cluster NGC 6819
Published by
LAP LAMBERT Academic Publishing Nov 2014, 2014
ISBN 10: 3659637149
ISBN 13: 9783659637148
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Taschenbuch
Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germany
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Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The evolution and energy production process of stars is dependent on their masses. Stars are observed to lose mass during their evolution along the Red Giant Branch (RGB). Therefore, by the time stars reach the Red Giant Clump (RGC), they are said to have undergone enormous mass loss. This may inturn affect the evolutionary path of these stars. Using the data from the Kepler open cluster, NGC 6819, the masses of stars along the RGB and RGC were obtained using the asteroseismic parameters (such as maximum pulsational frequency and large frequency separation). The age of the RGC stars was obtained using the age - metallicity relation. The mass loss mechanisms, amount of mass lost by stars from RGB to RGC, the effect of mass loss on the distribution of stars at the Clump are discussed in detail in this book.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 96 pp. Englisch. Seller Inventory # 9783659637148
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Mass Loss and Age of the RGC Stars in the Kepler Cluster NGC 6819
Published by
LAP LAMBERT Academic Publishing, 2014
ISBN 10: 3659637149
ISBN 13: 9783659637148
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Taschenbuch
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Taschenbuch. Condition: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - The evolution and energy production process of stars is dependent on their masses. Stars are observed to lose mass during their evolution along the Red Giant Branch (RGB). Therefore, by the time stars reach the Red Giant Clump (RGC), they are said to have undergone enormous mass loss. This may inturn affect the evolutionary path of these stars. Using the data from the Kepler open cluster, NGC 6819, the masses of stars along the RGB and RGC were obtained using the asteroseismic parameters (such as maximum pulsational frequency and large frequency separation). The age of the RGC stars was obtained using the age - metallicity relation. The mass loss mechanisms, amount of mass lost by stars from RGB to RGC, the effect of mass loss on the distribution of stars at the Clump are discussed in detail in this book. Seller Inventory # 9783659637148
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Mass Loss and Age of the RGC Stars in the Kepler Cluster NGC 6819
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LAP LAMBERT Academic Publishing, 2014
ISBN 10: 3659637149
ISBN 13: 9783659637148
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Taschenbuch. Condition: Neu. Mass Loss and Age of the RGC Stars in the Kepler Cluster NGC 6819 | Benard Nsamba (u. a.) | Taschenbuch | 96 S. | Englisch | 2014 | LAP LAMBERT Academic Publishing | EAN 9783659637148 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu. Seller Inventory # 104975662
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Mass Loss and Age of the RGC Stars in the Kepler Cluster NGC 6819
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