New discoveries of young stars revise our star formation history in the Taurus Molecular Cloud  

作　　者：Gregory J.Herczeg 

机构地区：[1]Kavli Institute for Astronomy and Astrophysics,Peking University,Beijing 100871,China [2]Department of Astronomy,School of Physics,Peking University,Beijing 100871,China

出　　处：《Science China(Physics,Mechanics & Astronomy)》2025年第4期263-264,共2页中国科学:物理学、力学、天文学(英文版)

摘　　要：As one of the nearest sites of low-mass star formation,the Taurus Molecular Cloud provides us with a foundation for how low-mass stars form and evolve.The members include T Tau,the namesake for the entire T Tauri class of stars,the famous HL Tau disk,and several of the most famous protostars.The cluster is not a single site of star formation,but a complicated combination of very young protostars,older generations of stars,along with gas and dust.

关 键 词：STARS Molecular CLOUD 

分 类 号：P15[天文地球—天文学]