張波

先後講授過恆星物理，恆星大氣物理，天體物理中的輻射機制、廣義相對論、核天體物理、電動力學、電動力學（II）等多門課程。

張波教授現已招收16屆全日制碩士研究生，已畢業32名，其中16名考取博士研究生。作為中科院國家天文台博士生導師，指導天文台博士生1名並已取得博士學位。作為理論物理專業博士生導師，目前指導博士生2名。

核天體物理是物理學與天體物理的重要交叉學科，其內容涉及天體物理學中恆星的演化、雙星的演化、星系的化學演化、物理學中的原子物理學、原子核物理學等多個學科，研究手段包括理論計算和天文觀測。事實上，宇宙中各種天體中的核合成是理論物理和原子核物理的天然實驗場。自20世紀90年代以來，隨著大口徑望遠鏡的投入使用，使得人們對暗弱天體的觀測成為可能，並積累了一批不同金屬丰度和不同演化階段的恆星的化學丰度資料，為恆星重元素核合成及中子俘獲元素丰度的研究提供了必要的天文觀測數據，也使得這方面的研究再次成為天體物理學的熱點課題。張波教授主要研究核天體物理中與恆星演化相關的中子俘獲元素的丰度和核合成問題，對它的研究既可了解自然界中各種原子核的來源，又可得到各種原子核性質方面的相關信息。其特色在於把基礎理論研究和實驗及觀測數據的唯象分析相結合，重點研究核天體物理中的新現象新物理，在某些關鍵點上取得進展。研究內容主要包括四個方面：

（1）AGB星s-過程核合成；

（2）鋇星系統軌道根數及s-過程元素丰度分佈規律；

（3）恆星中子俘獲元素丰度分佈及星系化學演化；

（4）r-過程核合成場所及元素丰度分佈規律。

1國家自然科學基金面上項目：貧金屬環境中子俘獲過程相關元素丰度分佈特徵及物理關聯的整體研究

（批准號：10973006，2010-2012，主持人：張波，主研人：李冀、崔文元、張江、楊大衛；40萬元）

2國家自然科學基金面上項目：鉛星和s+r星的產生原因及形成機制探究

（批准號：10673002，2007-2009，主持人：張波，主研人：李冀、楊大衛；26萬元）

3國家自然科學基金面上項目：AGB星s-過程核合成與中子輻照量分佈函數

（批准號：10373005，2004-2006，主持人：張波，主研人：楊大衛；25萬元）

4國家自然科學基金面上項目：中子俘獲元素的丰度分佈和星系化學演化

（批准號：19973002，2000-2002，主持人：張波，主研人：李冀、楊大衛；12萬元）

5國家自然科學基金面上項目：矮造父變星周期的變化與變星內部核合成

（批准號：19673008，1997-1999，主持人：楊大衛，主研人：張波；4萬元）

6國家自然科學基金天文聯合基金面上項目：銀盤恆星的化學丰度與運動學和年齡的關係

（批准號：10778616，2007-2009，主持人：李冀，主研人：張波、楊大衛；24萬元）

[1] A model for calculating the abundances of neutron -capture elements in metal-poor stars

The Astrophysical Journal, 1999, 513: 910-918

Zhang Bo, Li Ji, Zhang Caixia, Liang Yanchun, Peng Qiuhe

[2] Neutron Capture Elements in the s- and r-Process-Rich Stars: Constraints on Neutron-Capture Nucleosynthesis Processes

The Astrophysical Journal，2006,642:1075-1081

Zhang Bo, Ma Kun, Zhou Guide

[3] Investigation for the Puzzling Abundance Pattern of the Neutron-Capture Elements in the Ultra Metal-Poor Star: CS 30322-023

The Astrophysical Journal, 2007, 657:1037-1041

Cui Wenyuan, Zhang Bo, Ma Kun, Zhang Lu

[4] Investigation for the Enrichment Pattern of the Elements Abundances in r+s Star HE 0338-3945: A Special r-II Star？

The Astrophysical Journal, 2010, 708: 51-57

Cui Wenyuan, Zhang Jiang, Zhu Zizhong, Zhang Bo

[5] The oxygen abundance calibrations and N/O abundance ratios of 40000 SDSS star-forming galaxies

The Astrophysical Journal, 2006, 652:257-269

Liang Yanchun, Yin Shaoying，F.Hammer, Deng Licai，H.Flores, Zhang Bo

[6] The heavy-element abundances of AGB Stars and the angular conservation model of wind accretion for barium stars

Astronomy and Astrophysics,2000，363: 555-567

Liang Yanchun, Zhao Gang, Zhang Bo

[7] Orbital elements of barium stars formed through a wind accretion scenario.

Astronomy and Astrophysics,2000，363: 660-666

Liu Junhong, Zhang Bo, Liang Yanchun , Peng Qiuhe

[8] Chemical compositions of four barium stars.

Astronomy and Astrophysics,2003，397: 257-265

Liang Yanchun, Zhao Gang ,Chen Yuqin, Qiu Hong-mei, Zhang Bo

[9] Empirical strong-line oxygen abundance calibrations from galaxies with electron-temperature measurements

Astronomy and Astrophysics,2007, 462: 535-546

Yin Shaoying, Liang Yanchun，F.Hammer,J.Brinchmann, Zhang Bo, Deng Licai，H.Flores

[10] The origin of the lead-rich stars in the Galactic Halo: investigation of the model parameters for the s-process .

Monthly Notices of the Royal Astronomical Society, 2006,368:305-309

Cui Wenyuan, Zhang Bo

[11] Investigation of the single neutron exposure model for the s-process: the primary nature of the neutron source.

Monthly Notices of the Royal Astronomical Society, 2007, 375:1418-1422

Ma Kun, Cui Wenyuan, Zhang Bo

[12] Study of Isotopic Fractions and Abundances of the Neutron-capture Elements in HD175305

Monthly Notices of the Royal Astronomical Society, 2009, in press

Zhang Jiang, Cui Wenyuan, Zhang Bo

[13] Evolution of the distribution of neutron exposures in the Galaxy disc: an analytical model

Journal of Astronomy and Astrophysics, 2007, 28:1-12

Cui Wenyuan, Zhang Weijuan，Zhang Bo

[14]Two r-process components in ultra-metal-poor stars:the neutron-capture element distribution of CS 22892-052.

Astrophysics and Space Science, 2002, 280:325-336.

Zhang Bo, Li Ji, Wang Yuexiang, Zhang Yanxia, Liu Junhong, Peng Qiuhe

[15] The yields of r- process elements and chemical evolution of the Galaxy.

Astrophysics and Space Science, 2006, 306:33-39

Chen Zhe，Zhang Jiang，Chen Yanping，Cui Wenyuan，Zhang Bo

[16] Orbital elements of the mild and strong barium stars formed through a wind accretion scenario

Astrophysics and Space Science, 2008, 314: 351-359

Cui Wenyuan，Zhang Bo, Quan Yamin, Zhou Guide, Chen Yanping

[17] Abundances of heavy elements in ultra-metal poor star CS22892-52

= 極貧金屬星CS 22892-052的重元素丰度研究.

Science in China（A）,1999,42:401-406. =中國科學(A輯), 1998, 28:1102-1106.

Zhang Bo,Zhang Caixia, Li Ji, Liang Yanchun, Peng Qiuhe

[18] Correlativity of nucleosynthesis in low-mass AGB stars=

= 低質量 AGB 星核合成事件的相關性研究

Science in China（A）, 1996,39:1112-1120. =中國科學(A輯), 1996,26: 1050-1156.

Liu Yongxin，Zhang Bo,, Peng Qiuhe

[19] Inverse Correlation of abundances in AGB Stars.

Chinese Physics Letters, 1998, 15: 76-78.

Zhang Bo,Liu Junhong, Liang Yanchun, Peng Qiuhe

[20] Abundances of elements in metal-poor star HD 126238.

Chinese Physics Letters, 1999, 16.619-621.

Li Ji, Zhang Bo, Wei Guoqiang,Zhang Liping, , Peng Qiuhe

[21] Abundances distribution of slow-process main heavy elements in AGB stars.

Chinese Physics Letters 2003, 20.962-964.

Zhang Miaojing, Zhang Bo,Li Guanglie

[22] R-Process Nucleosynthesis and Galactic Chemical Evolution of the Ba Peak Elements.

Chinese Physics Letters, 2003,20：2084-2087.

Song Hanfeng, Zhang Bo, Zhang Jiang, Wu Haibin , Peng Qiuhe

[23] Neutron Capture Elements in the Double Enhenced Star HE1305-0007: a new s- and r-Process Paradigm.

Chinese Physics Letters, 2007,24：1417-1420.

Cui Wenyuan, Cui Dongnuan, Du Yunshuang, Zhang Bo

[24] Mass Fraction of C-Pocket in Metal-Poor AGB Stars and the Primary Nature of Neutron Source

Chinese Physics Letters, 2009,26：039701, 1-4

Cui Dongnuan, Geng Yuanyuan, Cui Wenyuan, Zhang Bo

[25] Galactic chemical evolution of the lighter neutron capture elements Sr,Y,Zr.

Chinese Journal of Astronomy and Astrophysics,2003,5:431-442.

Du Cui-hua，Zhang Bo, Song Hanfeng, Peng Qiuhe

[26]New variable stars discovered as by-product of the Beijing Astronomical Observatory Supernova survey

Chinese Journal of Astronomy and Astrophysics,2002,2:463-473.

Kong Minzhi，Qiu Yulei，Shen Chuanjian,Deng Jinsong,Zhang Bo

[27] A statistical model for predicting the average abundances patterns of the heavy elements in metal-poor-stars

Chinese Journal of Astronomy and Astrophysics,2002,2:429-440

Zhang Bo, Zhang Yan-xia,Li Ji, Peng Qiuhe

[28] The Distributions of Neutron Exposures in AGB stars and the Galaxy

Chinese Journal of Astronomy and Astrophysics,2007,7:224-233

Wen–YuanCui,Feng–HuaZhang,Wei–JuanZhang,LuZhang,BoZhang.

[29] Model of wind accretion in extrinsic AGB stars under conservation of total angular momentum

= 外賦AGB星星風吸積的角動量守恆模型.

Chinese Astronomy and Astrophysics,1999,23:189-194 =天文學報,1998,39:424-429.

Zhang Bo, Liu Junhong, Liang Yanchun, Peng Qiuhe

[30] A methed of evaluating abundances of heavy elements in metal-poor stars

= 一種研究貧金屬星重元素丰度分佈的方法.

Chinese Astronomy and Astrophysics, 2000,24:88-94= 天文學報,1999,40:256-262.

Zhang Bo,Li Ji, Zhang Caixia, Liang Yanchun , Peng Qiuhe

[31] The abundance distribution of Neutron-capture elements in metal Poor stars

= 貧金屬星中子俘獲元素丰度分佈

Chinese Astronomy and Astrophysics, 2001,25:298-304 =天文學報,2001,42:22-28.

Zhang Bo, Zhang Yanxia, Liu Junhong, Li Ji, Peng Qiuhe

[32] The nucleosynthesis of elements in low-mass AGB stars= 低質量 AGB 星重元素的核合成.

Chinese Astronomy and Astrophysics,1997,21:59-69= 天文學報,1996,37:243-253.

Wang Xinge, Zhang Bo, Peng Qiuhe

[33] Monte Carlo simulations of the orbital elements and abundances of Barium stars

= 鋇星系統軌道根數及丰度分佈的Monte-Carlo模擬計算.

Chinese Astronomy and Astrophysics,2003,27:292-302= 天文學報，2003，44:116-125.

Shi Weibin, Niu Ping, Zhang Bo, Liu Junhong, Peng Qiuhe

[34] Evolution of the s-element abundances of 3M asymptotic giant branch stars

= 3 MAGB 星表面重元素丰度的演化.

Chinese Astronomy and Astrophysics, 1998,22:49-55. =天文學報, 1997,38:232-238.

Zhang Bo, Chang Ruixiang, Peng Qiuhe

[35] A new formula for computing mean neutron exposure = 計算平均中子輻照量的新公式

Chinese Astronomy and Astrophysics, 2008, 32:369-379. =天文學報, 2008, 49: 133-143

Zhang Fenghua, Zhou Guide, Zhang Bo

[36] The color-magnitude relation of disk galaxies= 盤狀星系的顏色星等關係

Chinese Astronomy and Astrophysics, 2007, 31:236-243 =天文學報, 2007, 48: 11-17

Wu Haibin, Liu Chengze, Zhang Bo, Chang Ruixiang

[37] The overbundance of s-process elements in Ba stars through wind accretion

= 星風吸積引起的鋇星重元素超豐.

Chinese Astronomy and Astrophysics, 1997,21:453-460=天體物理學報,1997,17:284-290.

Chang Ruixiang, Zhang Bo, Peng Qiuhe

[38]The average abundance of heavy elements in metal poor stars in different metallicity ranges

=貧金屬星中子俘獲元素平均丰度的金屬丰度分區研究.

Chinese Astronomy and Astrophysics, 2001,25:187-193=天體物理學報,2000,20:277-284.

Zhang Yanxia, Zhang Bo, Li Ji, Liu Junhong, Peng Qiuhe

[39] Period variation of x-ray pulsars and Kelvin-Helmholtz instability at the accretion disk boundary

= X-射線脈衝星周期的變化與吸積盤的K-H不穩定性.

Chinese Astronomy and Astrophysics,1989,13:366-372 =天體物理學報,1989,9:244-250.

Zhang Bo, Ge Yunzao

[40] Nucleosynthesis of fluorine in low-mass AGB stars during the thermal pulse phase

= 小質量AGB星熱脈衝階段氟的核合成.

Chinese Astronomy and Astrophysics,1996,20:231-238= 天體物理學報,1996,16:58-64

Liu Yongxing, Zhang Bo, Peng Qiuhe

[41] Ba星星風吸積機制的再研究. 天體物理學報,1999,19:213-219. 梁艷春, 張波，彭秋和

[42]貧金屬星的表面元素丰度與慢中子俘獲過程. 高能物理與核物理,2003，27：304-308.張妙靜，張波，厲光烈

[43]太陽系元素丰度與AGB星慢中子俘獲元素. 高能物理與核物理,2003，27：978-983。張妙靜，張波，厲光烈

[44]貧金屬星的中子俘獲元素. 高能物理與核物理,2004，28：30-36.張妙靜，張波，厲光烈

[45] AGB星演化過程中的核合成. 原子核物理評論,2002,13：321-328. 張妙靜，張波，厲光烈

[46] AGB 星核合成理論的研究進展. 天文學進展,1996,14:275-285. 張波，常瑞香，彭秋和

[47]貧金屬星中子俘獲元素丰度. 天文學進展.2000,18:238-248. 張波，李冀，張彥霞，彭秋和

[48] AGB 星s-過程核合成相關問題的研究進展. 天文學進展 2006,24:54-61.張波，崔文元