中国科学院机构知识库网格
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Fast transition between classical and weak lined T Tauri stars due to external UV dissipation

文献类型:期刊论文

作者Li, J. Z.; Rector, T. A.
刊名NEW ASTRONOMY
出版日期2007-08-01
卷号12期号:6页码:441-445
关键词Stars : formation Stars : pre-main sequence Herbig-Haro objects ISM : jets and outflows
英文摘要The discovery of optical jets immersed in the strong UV radiation field of the Rosette Nebula sheds new light on, but meanwhile poses challenges to, the study of externally irradiated jets. The jet systems in the Rosette are found to have a high state of ionization and show unique features. In this paper, we investigate the evolutionary status of the jet-driving sources for young solar-like stars. To our surprise, these jet sources indicate unexpected near infrared properties with no excess emission. They are bathed in harsh external UV radiation such that evaporation leads to a fast dissipation of their circumstellar material. This could represent a transient phase of evolution of young solar-like stars between classical and weak lined T Tauri stars. Naked T Tauri stars formed in this way have indistinguishable evolutionary ages from those of classical T Tauri stars resulting from the same episode of star formation. However, it would be hard for such sources to be identified if they are not driving an irradiated jet in a photoionized medium. (C) 2007 Elsevier B.V. All rights reserved.
收录类别SCI
语种英语
WOS记录号WOS:000246728100002
源URL[http://ir.bao.ac.cn/handle/114a11/7272]  
专题国家天文台_应用天文研究部
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Univ Alaska, Anchorage, AK 99508 USA
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GB/T 7714
Li, J. Z.,Rector, T. A.. Fast transition between classical and weak lined T Tauri stars due to external UV dissipation[J]. NEW ASTRONOMY,2007,12(6):441-445.
APA Li, J. Z.,&Rector, T. A..(2007).Fast transition between classical and weak lined T Tauri stars due to external UV dissipation.NEW ASTRONOMY,12(6),441-445.
MLA Li, J. Z.,et al."Fast transition between classical and weak lined T Tauri stars due to external UV dissipation".NEW ASTRONOMY 12.6(2007):441-445.

入库方式: OAI收割

来源:国家天文台

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