Star-Formation Rates of Galaxies

·
· Cambridge Astrophysics 第 55 冊 · Cambridge University Press
電子書
318
頁數

關於這本電子書

Star-formation is one of the key processes that shape the current state and evolution of galaxies. This volume provides a comprehensive presentation of the different methods used to measure the intensity of recent or on-going star-forming activity in galaxies, discussing their advantages and complications in detail. It includes a thorough overview of the theoretical underpinnings of star-formation rate indicators, including topics such as stellar evolution and stellar spectra, the stellar initial mass function, and the physical conditions in the interstellar medium. The authors bring together in one place detailed and comparative discussions of traditional and new star-formation rate indicators, star-formation rate measurements in different spatial scales, and comparisons of star-formation rate indicators probing different stellar populations, along with the corresponding theoretical background. This is a useful reference for students and researchers working in the field of extragalactic astrophysics and studying star-formation in local and higher-redshift galaxies.

關於作者

Andreas Zezas is Associate Professor at the University of Crete. He studies the X-ray emission from galaxies and its connection with their current and past star-forming activity. He has co-authored over 200 refereed publications and has been awarded an ERC Consolidator grant.

Véronique Buat is Professor of Astrophysics at Aix-Marseille University and Senior Member of the Institut Universitaire de France. She works on large multi-wavelength galaxy surveys and develops models to study star formation and interstellar obscuration from the local to the distant universe.

為這本電子書評分

請分享你的寶貴意見。

閱讀資訊

智能手機和平板電腦
請安裝 Android 版iPad/iPhone 版「Google Play 圖書」應用程式。這個應用程式會自動與你的帳戶保持同步,讓你隨時隨地上網或離線閱讀。
手提電腦和電腦
你可以使用電腦的網絡瀏覽器聆聽在 Google Play 上購買的有聲書。
電子書閱讀器及其他裝置
如要在 Kobo 等電子墨水裝置上閱覽書籍,你需要下載檔案並傳輸到你的裝置。請按照說明中心的詳細指示,將檔案傳輸到支援的電子書閱讀器。