Spectral Energy Distribution for T Tauri Stars with a Debris Disk

被引:0
作者
N. Z. Ismailov
U. S. Valiev
机构
[1] N. Tusi Shamakhy Astrophysical Observatory of the Azerbaijan National Academy of Sciences,
[2] Batabat Astrophysical Observatory,undefined
[3] Nakhichevan Branch of the Azerbaijan National Academy of Sciences,undefined
来源
Astronomy Reports | 2022年 / 66卷
关键词
stars; circumstellar matter; pre-Main Sequence stars; infrared radiation; T Tauri variables;
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中图分类号
学科分类号
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页码:965 / 980
页数:15
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[1]  
Appenzeller I.(1989)Azerb Astron. Astrophys. Rev. 1 291-undefined
[2]  
Mundt R.(2004)undefined Astron. Astrophys. 424 603-undefined
[3]  
Jayawardhana R.(2003)undefined Astrophys. J. 592 282-undefined
[4]  
Mohanty S.(2003)undefined Astrophys. J. 582 1109-undefined
[5]  
Basri G.(2006)undefined Astrophys. J. 645 128-undefined
[6]  
White R. J.(2010)undefined Astrophy. J. 724 835-undefined
[7]  
Basri G.(2019)undefined Mon. Not. R. Astron. Soc. 482 698-undefined
[8]  
Padgett D. L.(2019)undefined Astron. Astrophys. 628 85-undefined
[9]  
Cieza L.(2021)undefined Astrophys. J. 913 123-undefined
[10]  
Stapelfeldt K. R.(2009)undefined Astrophys. J. 691 1265-undefined