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Chinese Academy of Sciences Institutional Repositories Grid
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CAS IR Grid
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新疆天文台 [3]
国家天文台 [2]
长春光学精密机械与物... [1]
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期刊论文 [5]
会议论文 [1]
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2024 [1]
2023 [1]
2021 [1]
2020 [1]
2011 [1]
2010 [1]
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The Population Synthesis of Wolf-Rayet Stars Involving Binary Merger Channels
期刊论文
OAI收割
Astrophysical Journal, 2024, 卷号: 969, 期号: 2, 页码: 11160
作者:
Zhuowen Li
;
Chunhua Zhu
;
Guoliang Lü
;
Lin Li
;
Helei Liu
  |  
收藏
  |  
浏览/下载:1/0
  |  
提交时间:2025/06/05
large-magellanic-cloud
spectroscopic multiplicity survey
common
envelope evolution
black-hole binaries
mass-loss rates
stellar
evolution
presupernova evolution
modern search
model grids
o-stars
Astronomy & Astrophysics
Molecules in the peculiar age-defying source IRAS 19312+1950
期刊论文
OAI收割
Astronomy & Astrophysics, 2023, 卷号: 669, 页码: A121
作者:
Qiu, Jian-Jie
;
Zhang, Yong
;
Nakashima, Jun-ichi
;
Zhang, Jiang-Shui
;
Koning, Nico
  |  
收藏
  |  
浏览/下载:1/0
  |  
提交时间:2024/06/23
ISM
molecules
circumstellar matter
line
identification
sio maser source
circumstellar envelopes
line survey
cologne
database
stellar-merger
h2o masers
emission
abundances
submillimeter
stars
Astronomy & Astrophysics
Galactic O-type Stars in LAMOST Data
期刊论文
OAI收割
The Astrophysical Journal Supplement Series, 2021, 卷号: 253, 期号: 2
作者:
Li,Guang-Wei
  |  
收藏
  |  
浏览/下载:13/0
  |  
提交时间:2021/12/06
O stars
Oe stars
Oef stars
Of stars
O dwarf stars
O giant stars
O subgiant stars
O supergiant stars
Spectroscopy
Spectroscopic binary stars
Two New Rapidly Rotating ON Stars Found with LAMOST
期刊论文
OAI收割
The Astrophysical Journal, 2020, 卷号: 888, 期号: 2
作者:
Li,Guang-Wei
;
Howarth,Ian D.
  |  
收藏
  |  
浏览/下载:18/0
  |  
提交时间:2020/03/10
Stellar rotation
O stars
A hybrid median filter for enhancing dim small point targets and its fast implementation (EI CONFERENCE)
会议论文
OAI收割
2011 International Conference on Multimedia and Signal Processing, CMSP 2011, May 14, 2011 - May 15, 2011, Guilin, Guangxi, China
Yang Q.
收藏
  |  
浏览/下载:24/0
  |  
提交时间:2013/03/25
Weak stars and middle altitude orbit satellites or high altitude orbit satellites are presented as dim point targets in images of astronomical observation. They have low intensity and occupy few pixels in image. In most situations
the background of sky is always ununiform and there exists pulse noises. Thus results in targets submerging in background noises and low signal noise ratio (SNR). Median filter is an effective method for removing pulse noise. But it can blur image after modifying gray of non-noise pixels when image has low SNR. A hybrid median filter algorithm is proposed to process low SNR dim point targets image. The newly proposed method can suppress the pulse noises
also can increase target $SNR$ and does not add extra fake targets. The time complexity of median filter is O(N2)(N is the widow size) and is difficult to implement in hardware. For quasi real time application
a fast implementation of our hybrid median filter is proposed to reduce the time complexity to O(N). Experimental results show that the newly proposed algorithm is superior to ordinary median filter and fast median filter by comparing visual effect and performance. 2011 IEEE.
The properties of a large sample of OH/IR stars, S stars and C-rich AGB stars
期刊论文
OAI收割
ASTROPHYSICS AND SPACE SCIENCE, 2010, 卷号: 330, 期号: 1, 页码: 23-36
作者:
Zhang, Hai-juan
;
Zhou, Jian-jun
;
Dong, Guo-liang
;
Esimbek, Jarken
;
Mu, Ji-mang
收藏
  |  
浏览/下载:22/0
  |  
提交时间:2015/08/25
O-rich (OH/IR) stars
S-stars
C-rich stars
Mass loss
Spectrum energy distributions