On the mass ejection and thermal pulses of an AGB star with an initial mass of 7-m-circle-dot | |
Jiang SY(蒋苏云); Huang RQ(黄润乾); Yuan YQ(袁永泉) | |
刊名 | ASTRONOMY & ASTROPHYSICS |
1995-01 | |
卷号 | 293期号:3页码:823-827 |
关键词 | STARS, AGE STARS, MASS LOSS STARS, INTERIORS |
ISSN号 | 0004-6361 |
产权排序 | 第一完成单位 |
英文摘要 | The mechanism driving the episode of large mass loss called superwind from an AGE star with initial mass of 7 M(circle dot) is studied by comparing the current luminosity of the star with its maximum luminosity set by the balance of several inward and outward acceleration mechanisms (gravity, radiation, rotation, and turbulent forces). The current luminosity during the AGE phase can exceed the maximum luminosity causing mass ejection from the AGE star. The periodic variation of the luminosity is in turn caused by variations in the energy output from the H-burning shelf, which are not related to the thermal pulses of the He-burning shell. The nature of the oscillatory behaviour of the H-burning shell is briefly investigated. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | WOLF-RAYET STARS ; EVOLUTIONARY MODELS ; VARIABLES ; ABUNDANCES ; ENRICHMENT ; GRIDS |
收录类别 | SCI |
原文出处 | http://adsabs.harvard.edu/abs/1995A%26A...293..823J |
语种 | 英语 |
WOS记录号 | WOS:A1995QD23400020 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/5138] |
专题 | 云南天文台_恒星物理研究组 |
作者单位 | Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming, P.R. China |
推荐引用方式 GB/T 7714 | Jiang SY,Huang RQ,Yuan YQ. On the mass ejection and thermal pulses of an AGB star with an initial mass of 7-m-circle-dot[J]. ASTRONOMY & ASTROPHYSICS,1995,293(3):823-827. |
APA | Jiang SY,Huang RQ,&Yuan YQ.(1995).On the mass ejection and thermal pulses of an AGB star with an initial mass of 7-m-circle-dot.ASTRONOMY & ASTROPHYSICS,293(3),823-827. |
MLA | Jiang SY,et al."On the mass ejection and thermal pulses of an AGB star with an initial mass of 7-m-circle-dot".ASTRONOMY & ASTROPHYSICS 293.3(1995):823-827. |
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