Tunable plasma narrow-band filter for ultrafast high-power lasers

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Dongjun Zhang ◽  
Ping Zhu ◽  
Xinglong Xie ◽  
Yan Liang ◽  
Qingwei Yang ◽  
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2008 ◽  
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M.I. Petelin ◽  
D.Yu Shchegolkov ◽  
V. Erckmann ◽  
B. Plaum ◽  
...  

2017 ◽  
Vol 9 (2) ◽  
pp. 1-8
Author(s):  
Chaolong Fang ◽  
Bo Dai ◽  
Qiao Xu ◽  
Qi Wang ◽  
Dawei Zhang

1998 ◽  
Vol 330 (2) ◽  
pp. 150-156 ◽  
Author(s):  
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Bl. Pantchev ◽  
P. Danesh ◽  
B. Zafirova ◽  
E. Karakoleva

1982 ◽  
Vol 72 (12) ◽  
pp. 1714 ◽  
Author(s):  
M. V. R. K. Murty ◽  
N. C. Das

1971 ◽  
Vol 83 ◽  
pp. 93 ◽  
Author(s):  
Torrence V. Johnson ◽  
Larry A. Lebofsky ◽  
Thomas B. McCord

2013 ◽  
Vol 33 (11) ◽  
pp. 1123003
Author(s):  
罗昕 Luo Xin ◽  
邹喜华 Zou Xihua ◽  
温坤华 Wen Kunhua ◽  
潘炜 Pan Wei ◽  
闫连山 Yan Lianshan ◽  
...  

2010 ◽  
Vol 22 (8) ◽  
pp. 1819-1822
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岳威 Yue Wei ◽  
洪冬梅 Hong Dongmei ◽  
刘国喜 Liu Guoxi ◽  
韩永昶 Han Yongchang ◽  
刘连泽 Liu Lianze ◽  
...  

1982 ◽  
Vol 99 ◽  
pp. 531-537
Author(s):  
Michael M. Shara ◽  
Anthony F. J. Moffat

A search to continuum magnitude B ∼ 21.5 (MB∼ −3) using a narrow band filter at λ4670å and a wide B-band filter has revealed 21 Wolf-Rayet star candidates in about half the giant Sb galaxy M31. Some weak-line WR stars, particularly WN subtypes, may have escaped detection. These numbers are compatible with the total number of luminous (i.e. massive) stars in M31. Eighteen of twenty confirmed candidate stars in M31 lie in the direction of 0B associations in the ring of prominent star formation 5–16 kpc from the center.


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