Possible Formation Scenarios of ZTF J153932.16+502738.8-A Gravitational Source Close to the Peak of LISA's Sensitivity
文献类型:期刊论文
作者 | Lu, Guoliang2,3; Zhu, Chunhua2,3; Wang, Zhaojun2,3; Liu, Helei2,3; Li, Lin2,3; Xie, Dian3; Liu, Jinzhong1 |
刊名 | ASTROPHYSICAL JOURNAL |
出版日期 | 2020-02-10 |
卷号 | 890期号:1页码:69 |
ISSN号 | 0004-637X |
关键词 | Close binary stars White dwarf stars Classical novae |
DOI | 10.3847/1538-4357/ab6bcc |
通讯作者 | Lu, Guoliang(guolianglv@xao.ac.cn) |
产权排序 | 3 |
英文摘要 | ZTF J153932.16+502738.8 (ZTFJ1539) is an eclipsing double-white-dwarf system with an orbital period of 6.91 minutes, and a significant source for LISA detection of gravitational waves. However, the massive white dwarf (WD), with a mass of about 0.61 M-circle dot, has a high effective temperature (48,900 K), and the lower-mass WD, with a mass of about 0.21 M-circle dot, has a low effective temperature (<10,000 K). This discrepancy challenges the popular theory of binary evolution. We investigate the formation of ZTFJ1539 via nova and Algol scenarios. Assuming that the massive WD in ZTFJ1539 just experiences a thermonuclear runaway, the nova scenario can explain the effective temperatures of the two WDs in ZTFJ1539. However, in order to enlarge a semi-detached orbit of about 4-5 minutes to a detached orbit of about 7 minutes, the nova scenario needs a much higher kick velocity of about 200 km s(-1) during nova eruption. The high kick velocity can result in a high eccentricity of about 0.2-0.6. The Algol scenario can also produce ZTFJ1539 if we take a high efficient parameter for ejecting the common envelope and enhance the mass-loss rate via stellar wind trigger by tidal effect. |
WOS关键词 | POPULATION SYNTHESIS ; WHITE-DWARFS ; EVOLUTION ; BINARIES ; MODELS ; EJECTA ; STARS ; TIDES |
资助项目 | National Natural Science Foundation of China[11863005] ; National Natural Science Foundation of China[11763007] ; National Natural Science Foundation of China[11803026] ; National Natural Science Foundation of China[11563008] ; National Natural Science Foundation of China[11473024] ; National Natural Science Foundation of China[11463005] ; National Natural Science Foundation of China[11503008] ; Tianshan Youth Project of Xinjiang[2017Q014] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP PUBLISHING LTD |
WOS记录号 | WOS:000522096700001 |
资助机构 | National Natural Science Foundation of China ; Tianshan Youth Project of Xinjiang |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/3466] |
专题 | 新疆天文台_光学天文与技术应用研究室 |
通讯作者 | Lu, Guoliang |
作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Xinjiang Observ, Urumqi 830011, Peoples R China 2.Xinjiang Univ, Ctr Theoret Phys, Urumqi 830046, Peoples R China 3.Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830046, Peoples R China |
推荐引用方式 GB/T 7714 | Lu, Guoliang,Zhu, Chunhua,Wang, Zhaojun,et al. Possible Formation Scenarios of ZTF J153932.16+502738.8-A Gravitational Source Close to the Peak of LISA's Sensitivity[J]. ASTROPHYSICAL JOURNAL,2020,890(1):69. |
APA | Lu, Guoliang.,Zhu, Chunhua.,Wang, Zhaojun.,Liu, Helei.,Li, Lin.,...&Liu, Jinzhong.(2020).Possible Formation Scenarios of ZTF J153932.16+502738.8-A Gravitational Source Close to the Peak of LISA's Sensitivity.ASTROPHYSICAL JOURNAL,890(1),69. |
MLA | Lu, Guoliang,et al."Possible Formation Scenarios of ZTF J153932.16+502738.8-A Gravitational Source Close to the Peak of LISA's Sensitivity".ASTROPHYSICAL JOURNAL 890.1(2020):69. |
入库方式: OAI收割
来源:新疆天文台
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