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STELLAR POPULATIONS
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ISBN13：9783527409181
出版社：JOHN WILEY & SONS;LTD
作者：RENZINI
出版日：2011/09/21
裝訂／頁數：精裝／320頁
定價
：NT$ 5890 元優惠價
：90 折 5301 元
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This only up-to-date reference on stellar populations and development models includes coverage of distant galaxies, chemical evolution and supernovae. Written by highly acclaimed authorities in the field, the text makes use of specific problems to reveal the "kitchen secrets".
作者簡介
Alvio Greggio held a professorship at the University of Bologna before he joined the European Southern Observatory (ESO) as Very Large Telescope program scientist, where he served until 2005; since then he is working at the National Institute of Astrophysics, INAF, in Italy. About 200 peer reviewed papers bear his name, making him one of the most cited scientists in his field.
Laura Greggio is Associate Astronomer at INAF. Her research focus is on stellar evolution and populations as well as supernovae.
Laura Greggio is Associate Astronomer at INAF. Her research focus is on stellar evolution and populations as well as supernovae.
目次
0. Introduction
1. Firm and less Firm outcomes of Stellar Evolution Theory
2. The Energetics of Stellar Populations
3. The Stellar Populations of Pixels and Frames (Observing resolved stellar populations)
4. Synthetic Color-Magnitude Diagrams
5. Age Dating Methods and their Applications (Globular clusters, Galactic Bulge, M31, Resolved Galaxies)
6. Stellar Population Synthesis
7. The Initial Mass Function (IMF)
8. Stellar Population Diagnostics of Galaxy Formation (From low to high, to very high redshifts)
9. Supernovae (Core collapse and thermonuclear supervovae and their rates)
10. Chemical Evolution of Galaxies, Clusters of Galaxies and the Whole Universe
1. Firm and less Firm outcomes of Stellar Evolution Theory
2. The Energetics of Stellar Populations
3. The Stellar Populations of Pixels and Frames (Observing resolved stellar populations)
4. Synthetic Color-Magnitude Diagrams
5. Age Dating Methods and their Applications (Globular clusters, Galactic Bulge, M31, Resolved Galaxies)
6. Stellar Population Synthesis
7. The Initial Mass Function (IMF)
8. Stellar Population Diagnostics of Galaxy Formation (From low to high, to very high redshifts)
9. Supernovae (Core collapse and thermonuclear supervovae and their rates)
10. Chemical Evolution of Galaxies, Clusters of Galaxies and the Whole Universe
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