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

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] 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, 943(2): https://doaj.org/article/c8793b10bc5b47519cdaaa51406f9940.
[2] Cui, Yingzhen, Meng, Xiangcun, Podsiadlowski, Philipp, Song, Ren. Hydrodynamical simulations for the common-envelope wind model for Type Ia supernovae. 2022, http://arxiv.org/abs/2210.07607.
[3] 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, 666: http://dx.doi.org/10.1051/0004-6361/202243759.
[4] 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, 515(2): 2747-2754, [5] 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, 22(12): 322-334, http://dx.doi.org/10.1088/1674-4527/ac9e92.
[6] Zeng, Yaotian, Liu, ZhengWei, Meng, Xiangcun, Han, Zhanwen. On the rotation properties of a post-explosion helium-star companion in Type Iax supernovae. 2022, http://arxiv.org/abs/2206.03522.
[7] Meng, Xiangcun, Luo, Yangpin. Hot subdwarfs from the surviving companions of the white dwarf + main-sequence channel of Type Ia supernovae. 2021, [8] Meng, XiangCun, Han, ZhanWen, Podsiadlowski, Philipp, Li, Jiao. Blue Large-Amplitude Pulsators: the Possible Surviving Companions of Type Ia Supernovae. 2020, http://arxiv.org/abs/2009.11059.
[9] 孟祥存. The C/O ratio of He-accreting carbon-oxygen white dwarf and type Ia supernovae. RAA. 2020, [10] Xiangcun Meng, Philipp Podsiadlowski. The common-envelope wind model for type Ia supernovae. Why galaxies care about AGB stars :. 2020, 470-471, http://dx.doi.org/10.1017/S1743921318006543.
[11] 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, 633: https://www.webofscience.com/wos/woscc/full-record/WOS:000506363000004.
[12] Meng Xiangcun. High-velocity feature as the indicator of the stellar population of Type Ia supernovae. 2019, http://arxiv.org/abs/1910.07131.
[13] 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, 482(4): 5651-5665, http://ir.ynao.ac.cn/handle/114a53/19677.
[14] 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.
[15] Cui, Xiao, Meng, XiangCun, Han, ZhanWen. Hydrogen and helium shell burning during white dwarf accretion. RESEARCHINASTRONOMYANDASTROPHYSICS[J]. 2018, 18(5): http://lib.cqvip.com/Qikan/Article/Detail?id=675462522.
[16] 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.
[17] Meng, XiangCun, Han, ZhanWen. Why Are Peculiar Type Ia Supernovae More Likely to Show the Signature of a Single-degenerate Model?. ASTROPHYSICALJOURNALLETTERS[J]. 2018, 855(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000427064600004.
[18] 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.
[19] 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.
[20] 孟祥存. The surviving companions in type Ia supernova remnants Li-Qing. RAA. 2017, [21] 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, 817(2): http://ir.bao.ac.cn/handle/114a11/5432.
[22] 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, 588: https://www.webofscience.com/wos/woscc/full-record/WOS:000373207800100.
[23] Meng, Xiangcun, Gao, Yan, Han, Zhanwen. SNe Ia as a cosmological probe. INTERNATIONAL JOURNAL OF MODERN PHYSICS D[J]. 2015, 24(14): http://www.irgrid.ac.cn/handle/1471x/1060394.
[24] Meng, Xiangcun, Han, Zhanwen. A pair of CO plus He white dwarfs as the progenitor of 2005E-like supernovae?. ASTRONOMY & ASTROPHYSICS[J]. 2015, 573: http://www.irgrid.ac.cn/handle/1471x/1048817.
[25] Meng, Xiangcun, Podsiadlowski, Philipp. THE BIRTH RATE OF SNe Ia FROM HYBRID CONe WHITE DWARFS. ASTROPHYSICAL JOURNAL LETTERS[J]. 2014, 789(2): http://www.irgrid.ac.cn/handle/1471x/1048782.
[26] 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.
[27] Chen, Xuefei, Han, Zhanwen, Meng, Xiangcun. Accreting carbon-oxygen white dwarfs at explosive C ignition. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY[J]. 2014, 438(4): 3358-3367, http://www.irgrid.ac.cn/handle/1471x/1048792.
[28] 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, 776(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000327216100049.
[29] Meng, Xiangcun, Podsiadlowski, Philipp. CONSTRAINING THE SPIN-DOWN TIMESCALE OF THE WHITE DWARF PROGENITORS OF TYPE Ia SUPERNOVAE. ASTROPHYSICAL JOURNAL LETTERS[J]. 2013, 778(2): http://ir.ynao.ac.cn/handle/114a53/9423.
[30] 孟祥存. Grids of rotating stellar models with masses between 1.0 and 3.0 Msolar. Research in Astronomy and Astrophysics. 2013, [31] Yang, Wuming, Bi, Shaolan, Meng, Xiangcun, Tian, Zhijia. EVOLUTION OF ROTATIONAL VELOCITIES OF A-TYPE STARS. ASTROPHYSICAL JOURNAL LETTERS[J]. 2013, 765(2): https://www.webofscience.com/wos/woscc/full-record/WOS:000315489100012.
[32] 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, 422(2): 1552-1561, http://dx.doi.org/10.1111/j.1365-2966.2012.20728.x.
[33] 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.
[34] 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, 414(2): 1769-1776, http://dx.doi.org/10.1111/j.1365-2966.2011.18509.x.
[35] 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.
[36] Meng XiangCun, Yang WuMing. The companion properties of SNe Ia from the single degenerate model. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY[J]. 2011, 54(12): 2296-2300, http://lib.cqvip.com/Qikan/Article/Detail?id=40074080.
[37] 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, 63(4): L31-L35, https://www.webofscience.com/wos/woscc/full-record/WOS:000299135600002.
[38] 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.
[39] 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, 11(8): 965-973, http://lib.cqvip.com/Qikan/Article/Detail?id=38851502.
[40] 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, [41] 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, 731(2): http://dx.doi.org/10.1088/2041-8205/731/2/L37.
[42] 孟祥存, 韩占文. 2012年参宿四会爆炸吗. 物理[J]. 2011, 40(4): 211-, http://lib.cqvip.com/Qikan/Article/Detail?id=37436592.
[43] Yang, Wuming, Meng, Xiangcun. Models of mu Her with asteroseismic constraints. NEW ASTRONOMY[J]. 2010, 15(4): 367-372, https://www.webofscience.com/wos/woscc/full-record/WOS:000274611200007.
[44] 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, 409(2): 873-879, http://dx.doi.org/10.1111/j.1365-2966.2010.17358.x.
[45] 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.
[46] Meng, X, Yang, W. Companion stars of Type Ia supernovae with different metallicities. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYnull. 2010, 401(2): 1118-1130, https://www.webofscience.com/wos/woscc/full-record/WOS:000273317300027.
[47] 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.
[48] 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.
[49] 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, 53(9): 1732-1738, https://www.webofscience.com/wos/woscc/full-record/WOS:000280810000022.
[50] Meng, XiangCun, Yang, WuMing, Li, ZhongMu. The cooling time of white dwarfs produced from type Ia supernovae. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2010, 10(9): 927-934, http://lib.cqvip.com/Qikan/Article/Detail?id=35278602.
[51] Meng, Xiangcun, Yang, Wuming. WD plus MS systems as the progenitor of SNe Ia. ASTROPHYSICS AND SPACE SCIENCE[J]. 2010, 329(1-2): 287-291, https://www.webofscience.com/wos/woscc/full-record/WOS:000282823200047.
[52] 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.
[53] Yang, Wuming, Meng, Xiangcun. Frequency Separation Variations of the Solar Low-Degree p-Modes. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN[J]. 2009, 61(6): 1399-1406, https://www.webofscience.com/wos/woscc/full-record/WOS:000273306300023.
[54] 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.
[55] Wang, Bo, Chen, Xuefei, Meng, Xiangcun, Han, Zhanwen. EVOLVING TO TYPE Ia SUPERNOVAE WITH SHORT DELAY TIMES. ASTROPHYSICAL JOURNAL[J]. 2009, 701(2): 1540-1546, http://www.irgrid.ac.cn/handle/1471x/1048658.
[56] 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, 61(6): 1251-1260, https://www.webofscience.com/wos/woscc/full-record/WOS:000273306300008.
[57] 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, 9(11): 1259-1269, http://lib.cqvip.com/Qikan/Article/Detail?id=32217967.
[58] 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, 8(1): 71-, [59] 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, 8(1): 63-70, http://lib.cqvip.com/Qikan/Article/Detail?id=26576476.
[60] 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 CENTURYnull. 2008, 379-382, http://www.irgrid.ac.cn/handle/1471x/1008001.
[61] 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, 27(6): 724-729, http://lib.cqvip.com/Qikan/Article/Detail?id=29385133.
[62] 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.
[63] Wu Bin, Meng Xiang-cun, Han Zhan-wen. The Formation of Black Hole Binaries. CHINESE ASTRONOMY AND ASTROPHYSICS. 2008, 32(1): 23-32, http://dx.doi.org/10.1016/j.chinastron.2008.01.007.
[64] 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, [65] Meng, XiangCun, Chen, XueFei, Tout, Christopher A, Han, ZhanWen. The relation between the critical accretion rate of progenitors of SNe Ia and metallicity. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS[J]. 2006, 6(4): 461-469, http://lib.cqvip.com/Qikan/Article/Detail?id=22601263.

   

（ 1 ） Ia 型超新星的公共包层星风模型的构建和应用, 主持, 国家级, 2015-01--2018-12
（ 2 ） Ia型超新星前身星的理论和观测对比研究, 主持, 部委级, 2015-01--2017-12
（ 3 ） Ia型超新星前身星, 主持, 国家级, 2016-01--2018-12
（ 4 ） 云南省中青年学术技术带头人后备人才, 主持, 省级, 2016-01--2018-12
（ 5 ） Ia型超新星研究, 主持, 省级, 2019-01--2023-12
（ 6 ） Ia型超新星公共包层星风模型的发展和应用, 主持, 国家级, 2020-01--2023-12
（ 7 ） 毫秒脉冲星双星研究, 主持, 部委级, 2021-01--2023-12

（1）A CE-wind model of type Ia supernovae   2016-11-18
（2）A common-envelope wind model for SNe Ia   2016-07-20
（3）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
（4）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