Mass Loss and Age of the RGC Stars in the Kepler Cluster NGC 6819

Benard Nsamba

ISBN 10: 3659637149 / ISBN 13: 9783659637148

Published by LAP LAMBERT Academic Publishing Nov 2014, 2014

About this Item

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

Bibliographic Details

• Title: Mass Loss and Age of the RGC Stars in the Kepler Cluster NGC 6819
• Publisher: LAP LAMBERT Academic Publishing Nov 2014
• Publication Date: 2014
• Language: English
• ISBN 10: 3659637149
• ISBN 13: 9783659637148
• Binding: Taschenbuch
• Condition: Neu
• Dimensions: 220W x 150H x 6D millimeters 220 millimeters width by 150 millimeters height by 6 millimeters depth
• Weight: 161 grams

About this title

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.

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