我关注的领域有恒星结构与演化、双星演化及特殊恒星的形成、Ia型超新星和致密天体吸积以及相关的大样本恒星演化。

070401-天体物理

恒星物理, Ia型超新星，致密天体

2005-09--2008-06   中国科学院云南天文台   博士
2002-09--2005-06   中国科学院云南天文台   硕士
1998-09--2002-06   河北师范大学   学士

博士研究生

博士学位

   

2015-04~现在, 中国科学院云南天文台, 研究员
2014-01~2015-04,中国科学院云南天文台, 副研究员
2011-11~2014-01,河南理工大学, 教师、副教授
2008-06~2011-10,河南理工大学, 教师、讲师

   

（1） 大样本恒星演化与特殊恒星形成, 二等奖, 国家级, 2013
（2） 双星演化与特殊恒星形成, 一等奖, 省级, 2012

   

[1] New Astronomy. 2024, 第 5 作者
[2] Research in Astronomy and Astrophysics. 2024, 第 2 作者
[3] XiangCun Meng, JuJia Zhang, Xulin Zhao, LiPing Li, XiaoFeng Wang. Environments of Type Ia Supernovae with Different Relative Equivalent Widths of the Si ii Feature in Their Spectra. THE ASTROPHYSICAL JOURNAL[J]. 2023, 第 1 作者943(2): https://doaj.org/article/c8793b10bc5b47519cdaaa51406f9940.
[4] The Astrophysical Journal Letters. 2023, 第 2 作者
[5] Cui, Yingzhen, Meng, Xiangcun, Podsiadlowski, Philipp, Song, Ren. Hydrodynamical simulations for the common-envelope wind model for Type Ia supernovae. 2022, 第 2 作者http://arxiv.org/abs/2210.07607.
[6] Zhao, Weitao, Meng, Xiangcun, Cui, Yingzheng, Liu, ZhengWei. A robust model for the origin of optical quasi-periodic variability in supersoft X-ray sources. ASTRONOMY & ASTROPHYSICS[J]. 2022, 第 2 作者666: http://dx.doi.org/10.1051/0004-6361/202243759.
[7] Cui, Yingzhen, Meng, Xiangcun. The viability of the optically thick wind model in accreting white dwarfs at high accretion rates. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2022, 第 2 作者515(2): 2747-2754, 
[8] Lan, ShunYi, Ji, KaiFan, Meng, XiangCun. Machine Learning to Search for Accreting Neutron Star Binary Candidates Using Chinese Space Station Telescope Photometric System. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2022, 第 3 作者  通讯作者  22(12): 322-334, http://dx.doi.org/10.1088/1674-4527/ac9e92.
[9] Zeng, Yaotian, Liu, ZhengWei, Meng, Xiangcun, Han, Zhanwen. On the rotation properties of a post-explosion helium-star companion in Type Iax supernovae. 2022, 第 3 作者http://arxiv.org/abs/2206.03522.
[10] Meng, Xiangcun, Luo, Yangpin. Hot subdwarfs from the surviving companions of the white dwarf + main-sequence channel of Type Ia supernovae. 2021, 第 1 作者
[11] 孟祥存. The C/O ratio of He-accreting carbon-oxygen white dwarf and type Ia supernovae. RAA. 2020, 第 1 作者
[12] Meng, XiangCun, Han, ZhanWen, Podsiadlowski, Philipp, Li, Jiao. Blue Large-Amplitude Pulsators: the Possible Surviving Companions of Type Ia Supernovae. 2020, 第 1 作者http://arxiv.org/abs/2009.11059.
[13] Xiangcun Meng, Philipp Podsiadlowski. The common-envelope wind model for type Ia supernovae. Why galaxies care about AGB stars :. 2020, 第 1 作者470-471, http://dx.doi.org/10.1017/S1743921318006543.
[14] Meng, XiangCun, Han, ZhanWen, Podsiadlowski, Philipp, Li, Jiao. Blue Large-amplitude Pulsators: The Possible Surviving Companions of Type Ia Supernovae. ASTROPHYSICAL JOURNAL[J]. 2020, 第 1 作者  通讯作者  903(2): http://dx.doi.org/10.3847/1538-4357/abbb8e.
[15] Song, Ren, Meng, Xiangcun, Podsiadlowski, Philipp, Cui, Yingzhen. Structure of a massive common envelope in the common-envelope wind model for Type Ia supernovae. ASTRONOMY & ASTROPHYSICS[J]. 2020, 第 2 作者633: https://www.webofscience.com/wos/woscc/full-record/WOS:000506363000004.
[16] Meng Xiangcun. High-velocity feature as the indicator of the stellar population of Type Ia supernovae. 2019, 第 1 作者http://arxiv.org/abs/1910.07131.
[17] Meng, Xiangcun, Li, Jiao. Subdwarf B stars as possible surviving companions in Type Ia supernova remnants. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2019, 第 1 作者  通讯作者  482(4): 5651-5665, http://ir.ynao.ac.cn/handle/114a53/19677.
[18] Hc, Xiang, Meng, XiangCun, Chen, HaiLiang. Formation of accreting millisecond X-ray pulsars. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2019, 第 2 作者19(8): http://lib.cqvip.com/Qikan/Article/Detail?id=84848776504849574856484853.
[19] 贺祥. Formation of accreting millisecond X-ray pulsars. 天文和天体物理学研究:英文版[J]. 2019, 45-55, http://lib.cqvip.com/Qikan/Article/Detail?id=84848776504849574856484853.
[20] Meng, XiangCun. High-velocity Feature as the Indicator of the Stellar Population of Type Ia Supernovae. ASTROPHYSICAL JOURNAL[J]. 2019, 第 1 作者  通讯作者  886(1): 
[21] Cui, Xiao, Meng, XiangCun, Han, ZhanWen. Hydrogen and helium shell burning during white dwarf accretion. RESEARCHINASTRONOMYANDASTROPHYSICS[J]. 2018, 第 2 作者18(5): http://lib.cqvip.com/Qikan/Article/Detail?id=675462522.
[22] Meng, X, Podsiadlowski, Ph. Do SN 2002cx-like and SN Ia-CSM Objects Share the Same Origin?. ASTROPHYSICAL JOURNAL[J]. 2018, 861(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000438684300007.
[23] Meng, XiangCun, Han, ZhanWen. Why Are Peculiar Type Ia Supernovae More Likely to Show the Signature of a Single-degenerate Model?. ASTROPHYSICALJOURNALLETTERS[J]. 2018, 第 1 作者  通讯作者  855(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000427064600004.
[24] Chen Liqing, Meng Xiangcun, Han Zhanwen. The surviving companions in type la supernova remnants. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2017, 第 2 作者17(8): 83-1, http://sciencechina.cn/gw.jsp?action=detail.jsp&internal_id=6041040&detailType=1.
[25] Meng, X, Podsiadlowski, Ph. A common-envelope wind model for Type Ia supernovae - I. Binary evolution and birth rate. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2017, 469(4): 4763-4787, https://www.webofscience.com/wos/woscc/full-record/WOS:000406837900073.
[26] Meng, X, Zhang, J, Han, Z. A Polarization Sequence for Type Ia Supernovae?. ASTROPHYSICAL JOURNAL[J]. 2017, 841(1): http://ir.ynao.ac.cn/handle/114a53/10085.
[27] 孟祥存. The surviving companions in type Ia supernova remnants Li-Qing. RAA. 2017, 第 1 作者
[28] Chen, LiQing, Meng, XiangCun, Han, ZhanWen. The surviving companions in type Ia supernova remnants. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2017, 第 2 作者17(8): https://www.webofscience.com/wos/woscc/full-record/WOS:000416068900007.
[29] Zhang, JuJia, Wang, XiaoFeng, Sasdelli, Michele, Zhang, TianMeng, Liu, ZhengWei, Mazzali, Paolo A, Meng, XiangCun, Maeda, Keiichi, Chen, JunCheng, Huang, Fang, Zhao, XuLin, Zhang, KaiCheng, Zhai, Qian, Pian, Elena, Wang, Bo, Chang, Liang, Yi, WeiMin, Wang, ChuanJun, Wang, XueLi, Xin, YuXin, Wang, JianGuo, Lun, BaoLi, Zheng, XiangMing, Zhang, XiLiang, Fan, YuFeng, Bai, JinMing. A LUMINOUS PECULIAR TYPE IA SUPERNOVA SN 2011HR: MORE LIKE SN 1991T OR SN 2007if?. ASTROPHYSICAL JOURNAL[J]. 2016, 第 7 作者817(2): http://ir.bao.ac.cn/handle/114a11/5432.
[30] Meng, Xiangcun, Han, Zhanwen. The X-ray/radio and UV luminosity expected from symbiotic systems as the progenitor of SNe Ia. ASTRONOMY & ASTROPHYSICS[J]. 2016, 第 1 作者  通讯作者  588: https://www.webofscience.com/wos/woscc/full-record/WOS:000373207800100.
[31] Zhang, JuJia, Wang, XiaoFeng, Sasdelli, Michele, Zhang, TianMeng, Liu, ZhengWei, Mazzali, Paolo A, Meng, XiangCun, Maeda, Keiichi, Chen, JunCheng, Huang, Fang, Zhao, XuLin, Zhang, KaiCheng, Zhai, Qian, Pian, Elena, Wang, Bo, Chang, Liang, Yi, WeiMin, Wang, ChuanJun, Wang, XueLi, Xin, YuXin, Wang, JianGuo, Lun, BaoLi, Zheng, XiangMing, Zhang, XiLiang, Fan, YuFeng, Bai, JinMing. A LUMINOUS PECULIAR TYPE IA SUPERNOVA SN 2011HR: MORE LIKE SN 1991T OR SN 2007if?. ASTROPHYSICAL JOURNAL[J]. 2016, 第 7 作者817(2): http://ir.bao.ac.cn/handle/114a11/5432.
[32] Zhou, WeiHong, Wang, Bo, Meng, XiangCun, Liu, DongDong, Zhao, Gang. Binary population synthesis for the core-degenerate scenario of type Ia supernova progenitors. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2015, 第 3 作者15(10): 1701-1712, http://ir.bao.ac.cn/handle/114a11/5554.
[33] Meng, Xiangcun, Gao, Yan, Han, Zhanwen. SNe Ia as a cosmological probe. INTERNATIONAL JOURNAL OF MODERN PHYSICS D[J]. 2015, 第 1 作者  通讯作者  24(14): http://www.irgrid.ac.cn/handle/1471x/1060394.
[34] Meng, Xiangcun, Han, Zhanwen. A pair of CO plus He white dwarfs as the progenitor of 2005E-like supernovae?. ASTRONOMY & ASTROPHYSICS[J]. 2015, 第 1 作者  通讯作者  573: http://www.irgrid.ac.cn/handle/1471x/1048817.
[35] Meng, Xiangcun, Podsiadlowski, Philipp. THE BIRTH RATE OF SNe Ia FROM HYBRID CONe WHITE DWARFS. ASTROPHYSICAL JOURNAL LETTERS[J]. 2014, 第 1 作者  通讯作者  789(2): http://www.irgrid.ac.cn/handle/1471x/1048782.
[36] Wang, B, Meng, X, Liu, D D, Liu, Z W, Han, Z. THE HYBRID CONe WD plus He STAR SCENARIO FOR THE PROGENITORS OF TYPE Ia SUPERNOVAE. ASTROPHYSICAL JOURNAL LETTERS[J]. 2014, 794(2): http://www.irgrid.ac.cn/handle/1471x/1048775.
[37] Chen, Xuefei, Han, Zhanwen, Meng, Xiangcun. Accreting carbon-oxygen white dwarfs at explosive C ignition. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2014, 第 3 作者438(4): 3358-3367, http://www.irgrid.ac.cn/handle/1471x/1048792.
[38] Yang, Wuming, Bi, Shaolan, Meng, Xiangcun, Liu, Zhie. THE EFFECTS OF ROTATION ON THE MAIN-SEQUENCE TURNOFF OF INTERMEDIATE-AGE MASSIVE STAR CLUSTERS. ASTROPHYSICAL JOURNAL[J]. 2013, 第 3 作者776(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000327216100049.
[39] Meng, Xiangcun, Podsiadlowski, Philipp. CONSTRAINING THE SPIN-DOWN TIMESCALE OF THE WHITE DWARF PROGENITORS OF TYPE Ia SUPERNOVAE. ASTROPHYSICAL JOURNAL LETTERS[J]. 2013, 第 1 作者778(2): http://ir.ynao.ac.cn/handle/114a53/9423.
[40] 孟祥存. Grids of rotating stellar models with masses between 1.0 and 3.0 Msolar. Research in Astronomy and Astrophysics. 2013, 第 1 作者
[41] Yang, Wuming, Bi, Shaolan, Meng, Xiangcun, Tian, Zhijia. EVOLUTION OF ROTATIONAL VELOCITIES OF A-TYPE STARS. ASTROPHYSICAL JOURNAL LETTERS[J]. 2013, 第 3 作者765(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000315489100012.
[42] Yang, Wuming, Meng, Xiangcun, Bi, Shaolan, Tian, Zhijia, Liu, Kang, Li, Tanda, Li, Zhongmu. Characteristics of solar-like oscillations of secondary red-clump stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2012, 第 2 作者422(2): 1552-1561, http://dx.doi.org/10.1111/j.1365-2966.2012.20728.x.
[43] Meng, X, Yang, W. The birth rate of supernovae from double-degenerate and core-degenerate systems. ASTRONOMY & ASTROPHYSICS[J]. 2012, 543: http://ir.ynao.ac.cn/handle/114a53/9431.
[44] Yang, Wuming, Li, Zhongmu, Meng, Xiangcun, Bi, Shaolan. Characteristics of solar-like oscillations of clusters simulated by stellar population synthesis. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2011, 第 3 作者414(2): 1769-1776, http://dx.doi.org/10.1111/j.1365-2966.2011.18509.x.
[45] Meng, X C, Yang, W M. The correlation between C/O ratio, metallicity, and the initial WD mass for SNe Ia. ASTRONOMY & ASTROPHYSICS[J]. 2011, 531: https://www.webofscience.com/wos/woscc/full-record/WOS:000293017700065.
[46] Meng XiangCun, Yang WuMing. The companion properties of SNe Ia from the single degenerate model. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY[J]. 2011, 第 1 作者  通讯作者  54(12): 2296-2300, http://lib.cqvip.com/Qikan/Article/Detail?id=40074080.
[47] Meng, Xiang Cun, Li, Zhong Mu, Yang, Wu Ming. The Effect of Metallicity on the Delay-Time Distribution of Type Ia Supernova. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN[J]. 2011, 第 1 作者  通讯作者  63(4): L31-L35, https://www.webofscience.com/wos/woscc/full-record/WOS:000299135600002.
[48] Meng, X C, Chen, W C, Yang, W M, Li, Z M. The birth rate of subluminous and overluminous type Ia supernovae. ASTRONOMY & ASTROPHYSICS[J]. 2011, 525: https://www.webofscience.com/wos/woscc/full-record/WOS:000285193700059.
[49] Meng, XiangCun, Yang, WuMing. Binary population synthesis study of the supersoft X-ray phase of single degenerate type Ia supernova progenitors. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2011, 第 1 作者  通讯作者  11(8): 965-973, http://lib.cqvip.com/Qikan/Article/Detail?id=38851502.
[50] 孟祥存. 星周盘对Ia型超新星前身星演化的影响. 河南理工大学学报. 2011, 第 1 作者
[51] Yang, Wuming, Meng, Xiangcun, Bi, Shaolan, Tian, Zhijia, Li, Tanda, Liu, Kang. THE CONTRIBUTIONS OF INTERACTIVE BINARY STARS TO DOUBLE MAIN-SEQUENCE TURNOFFS AND DUAL RED CLUMP OF INTERMEDIATE-AGE STAR CLUSTERS. ASTROPHYSICAL JOURNAL LETTERS[J]. 2011, 第 2 作者731(2): http://dx.doi.org/10.1088/2041-8205/731/2/L37.
[52] 孟祥存, 韩占文. 2012年，参宿四会爆炸吗？. 物理[J]. 2011, 第 1 作者40(4): 211, http://www.wuli.ac.cn/cn/article/id/31970.
[53] Yang, Wuming, Meng, Xiangcun. Models of mu Her with asteroseismic constraints. NEW ASTRONOMY[J]. 2010, 第 2 作者15(4): 367-372, https://www.webofscience.com/wos/woscc/full-record/WOS:000274611200007.
[54] Yang, Wuming, Meng, Xiangcun, Li, Zhongmu. The effects of stellar population synthesis on the distributions of the asteroseismic observables nu(max) and Delta nu of red-clump stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2010, 第 2 作者409(2): 873-879, http://dx.doi.org/10.1111/j.1365-2966.2010.17358.x.
[55] Meng, X, Yang, W, Geng, X. Is SN 2006X from a WD plus MS system with optically thick wind?. NEW ASTRONOMY[J]. 2010, 15(4): 343-345, https://www.webofscience.com/wos/woscc/full-record/WOS:000274611200002.
[56] Meng, X, Yang, W. Companion stars of Type Ia supernovae with different metallicities. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2010, 401(2): 1118-1130, https://www.webofscience.com/wos/woscc/full-record/WOS:000273317300027.
[57] Meng, X, Yang, W. A COMPREHENSIVE PROGENITOR MODEL FOR SNe Ia. ASTROPHYSICAL JOURNAL[J]. 2010, 710(2): 1310-1323, https://www.webofscience.com/wos/woscc/full-record/WOS:000274233300030.
[58] Meng, X, Yang, W. The envelope mass of red giant donors in type Ia supernova progenitors. ASTRONOMY & ASTROPHYSICS[J]. 2010, 516: https://www.webofscience.com/wos/woscc/full-record/WOS:000280275400062.
[59] Meng XiangCun, Yang WuMing, Li ZhongMu. The initial and final state of SNe Ia from the single degenerate model. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY[J]. 2010, 第 1 作者  通讯作者  53(9): 1732-1738, https://www.webofscience.com/wos/woscc/full-record/WOS:000280810000022.
[60] Meng, XiangCun, Yang, WuMing, Li, ZhongMu. The cooling time of white dwarfs produced from type Ia supernovae. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2010, 第 1 作者  通讯作者  10(9): 927-934, http://lib.cqvip.com/Qikan/Article/Detail?id=35278602.
[61] Meng, Xiangcun, Yang, Wuming. WD plus MS systems as the progenitor of SNe Ia. ASTROPHYSICS AND SPACE SCIENCE[J]. 2010, 第 1 作者  通讯作者  329(1-2): 287-291, https://www.webofscience.com/wos/woscc/full-record/WOS:000282823200047.
[62] Meng, X, Chen, X, Han, Z. A single-degenerate channel for the progenitors of Type Ia supernovae with different metallicities. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2009, 395(4): 2103-2116, http://www.irgrid.ac.cn/handle/1471x/1048663.
[63] Yang, Wuming, Meng, Xiangcun. Frequency Separation Variations of the Solar Low-Degree p-Modes. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN[J]. 2009, 第 2 作者61(6): 1399-1406, https://www.webofscience.com/wos/woscc/full-record/WOS:000273306300023.
[64] Wang, B, Meng, X, Chen, X, Han, Z. The helium star donor channel for the progenitors of Type Ia supernovae. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2009, 395(2): 847-854, http://www.irgrid.ac.cn/handle/1471x/1048664.
[65] Wang, Bo, Chen, Xuefei, Meng, Xiangcun, Han, Zhanwen. EVOLVING TO TYPE Ia SUPERNOVAE WITH SHORT DELAY TIMES. ASTROPHYSICAL JOURNAL[J]. 2009, 第 3 作者701(2): 1540-1546, http://www.irgrid.ac.cn/handle/1471x/1048658.
[66] Meng, Xiangcun, Yang, Wuming, Geng, Xuemin. WD plus MS Systems as Progenitors of Type Ia Supernovae with Different Metallicities. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN[J]. 2009, 第 1 作者  通讯作者  61(6): 1251-1260, https://www.webofscience.com/wos/woscc/full-record/WOS:000273306300008.
[67] Meng, XiangCun, Chen, XueFei, Han, ZhanWen, Yang, WuMing. Color excesses of type Ia supernovae from the single-degenerate channel model. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2009, 第 1 作者  通讯作者  9(11): 1259-1269, http://lib.cqvip.com/Qikan/Article/Detail?id=32217967.
[68] Bo Wang, XiangCun Meng, XiaoFeng Wang, ZhanWen Han. Distribution of 56Ni Yields of Type Ia Supernovae and its Implication for Progenitors. CHINESE ASTRONOMY AND ASTROPHYSICS[J]. 2008, 第 2 作者8(1): 71, 
[69] Meng Xiangcun, Chen Xuefei, Han Zhanwen. The single degenerate channel for the progenitors of Type Ia supernovae. IAU SYMPOSIUM PROCEEDINGS SERIES - ART OF MODELLING STARS IN THE 21ST CENTURY. 2008, 第 1 作者4(252): 379-382, http://www.irgrid.ac.cn/handle/1471x/1008001.
[70] Wen Guo, FengHui Zhang, XiangCun Meng, ZhongMu Li, ZhanWen Han. Model-synthesized rate of Type Ia Supernovae and its influence on the chemical enrichment of the ISM. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS[J]. 2008, 第 3 作者8(1): 63-70, http://lib.cqvip.com/Qikan/Article/Detail?id=26576476.
[71] Meng Xiangcun, Chen Xuefei, Han Zhanwen, Deng L, Chan KL. The single degenerate channel for the progenitors of Type Ia supernovae. ART OF MODELLING STARS IN THE 21ST CENTURY. 2008, 第 1 作者379-382, http://www.irgrid.ac.cn/handle/1471x/1008001.
[72] 孟祥存, 杨伍明. 双星演化对Ia型超新星伴星结构的影响. 河南理工大学学报：自然科学版[J]. 2008, 第 1 作者27(6): 724-729, http://lib.cqvip.com/Qikan/Article/Detail?id=29385133.
[73] Meng, X, Chen, X, Han, Z. Initial-final mass relationship for stars of different metallicities. ASTRONOMY & ASTROPHYSICS[J]. 2008, 487(2): 625-635, http://dx.doi.org/10.1051/0004-6361:20078841.
[74] Wu Bin, Meng Xiang-cun, Han Zhan-wen. The Formation of Black Hole Binaries. CHINESE ASTRONOMY AND ASTROPHYSICS. 2008, 第 2 作者32(1): 23-32, http://dx.doi.org/10.1016/j.chinastron.2008.01.007.
[75] Meng, Xiangcun, Chen, Xuefei, Han, Zhanwen. The impact of type Ia supernova explosions on the companion in a binary system. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN[J]. 2007, 第 1 作者  通讯作者  59(4): 835-840, http://www.irgrid.ac.cn/handle/1471x/1048634.
[76] 孟祥存. The Impact of Type Ia Supernova Explosions on the Companions in a Binary System. Publications of the Astronomical Society of Japan. 2007, 第 1 作者
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（ 1 ） Ia 型超新星的公共包层星风模型的构建和应用, 负责人, 国家任务, 2015-01--2018-12
（ 2 ） Ia型超新星前身星的理论和观测对比研究, 负责人, 中国科学院计划, 2015-01--2017-12
（ 3 ） Ia型超新星前身星, 负责人, 国家任务, 2016-01--2018-12
（ 4 ） 云南省中青年学术技术带头人后备人才, 负责人, 地方任务, 2016-01--2018-12
（ 5 ） Ia型超新星研究, 负责人, 地方任务, 2019-01--2023-12
（ 6 ） Ia型超新星公共包层星风模型的发展和应用, 负责人, 国家任务, 2020-01--2023-12
（ 7 ） 毫秒脉冲星双星研究, 负责人, 中国科学院计划, 2021-01--2023-12
（ 8 ） Ia型超新星及相关特殊天体研究, 负责人, 国家任务, 2024-01--2028-12
（ 9 ） Ia型超新星研究, 负责人, 地方任务, 2024-03--2027-02

（1）BLAPs: the probable surviving companion of type Ia supernovae   2023-09-11
（2）The common-envelope wind model for type Ia supernovae   2018-08-19
（3）A CE-wind model of type Ia supernovae   2016-11-18
（4）A common-envelope wind model for SNe Ia   2016-07-20
（5）Ia型超新星爆炸机制   第七届热亚矮星及相关天体国际会议   孟祥存   2015-07-19
（6）A CE-wind Single-Degenerate model for SNe Ia   2014落基山下的恒星探戈   Xiangcun Meng, Philipp Podsiadlowski   2014-04-26

已指导学生

贺祥  硕士研究生  070401-天体物理  

陈俐鲭  硕士研究生  070401-天体物理  

现指导学生

宋仁  硕士研究生  070401-天体物理  

赵伟涛  硕士研究生  070401-天体物理  

崔英朕  博士研究生  070401-天体物理