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課程名稱 |
天文物理二
ASTROPHYSICS(Ⅱ) |
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開課學期 |
96-2 |
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授課對象 |
理學院 天文物理研究所 |
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授課教師 |
賀曾樸 |
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課號 |
AsPhys7011 |
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課程識別碼 |
244 M1120 |
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班次 |
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學分 |
4 |
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全/半年 |
半年 |
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必/選修 |
必帶 |
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上課時間 |
星期一7,8(14:20~16:20)星期五3,4(10:20~12:10) |
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上課地點 |
新物618新物618 |
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備註 |
總人數上限：20人 |
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課程簡介影片 |
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核心能力關聯 |
核心能力與課程規劃關聯圖 |
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課程大綱
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課程概述 |
Course contents for Astrophysics II (2008 Spring semester)
1) Galactic dynamics. The motions of gas and stars in our Galaxy
and individual galaxies will be discussed. We start with the
morphological classifications of galaxies, then explain the
origin of the spiral patterns in our Galaxy and other galaxies.
There will be discussions of related topics such as the rotation
speed and the gravitational potential field of a disk galaxy
2) Interstellar medium. The atomic and molecular processes of
the gas in space will be discussed. Students will be introduced
to the concepts of cooling and heating of gas in space. We
will learn about interactions between gas and solid materials
(interstellar dust grains) in space. There will be a brief
> introduction to the heoretical aspects of star formation.
> 3) Extragalactic astronomy. Golbal characteristics of various types
> of galaxies will be discussed. The lectures will focus on
> (i) the britenss distributions and kinematics of galaxies,
> (ii) the various activities in galaxies, and (iii) the interactions
> between galaxies. Students will learn about the methods for
> distance estimation of the galaxies that are the foundations
> of the Hubble's law.
> ?
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課程目標 |
Course contents for Astrophysics II (2008 Spring semester)
> (NTU Institite of Astrophysics #2440)
>
> 1) Galactic dynamics. The motions of gas and stars in our Galaxy
> and individual galaxies will be discussed. We start with the
> morphological classifications of galaxies, then explain the
> origin of the spiral patterns in our Galaxy and other galaxies.
> There will be discussions of related topics such as the rotation
> speed and the gravitational potential field of a disk galaxy
> 2) Interstellar medium. The atomic and molecular processes of
> the gas in space will be discussed. Students will be introduced
> to the concepts of cooling and heating of gas in space. We
> will learn about interactions between gas and solid materials
> (interstellar dust grains) in space. There will be a brief
> introduction to the theoretical aspects of star formation.
> 3) Extragalactic astronomy. Golbal characteristics of various types
> of galaxies will be discussed. The lectures will focus on
> (i) the britenss distributions and kinematics of galaxies,
> (ii) the various activities in galaxies, and (iii) the interactions
> between galaxies. Students will learn about the methods for
> distance estimation of the galaxies that are the foundations
> of the Hubble's law.
> ?
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課程要求 |
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預期每週課後學習時數 |
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Office Hours |
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指定閱讀 |
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參考書目 |
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評量方式
(僅供參考) |
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