J1640 총13명이 열람하였으며, 0개의 리뷰가 있습니다.
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몰운대(20141230)
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펄사 쌍성 J1640–224, J1713–0747은 광도가 없는 거대 응집체(태양질량의 약 2.4×10^7배)가 태양으로부터 약 2.3천 광년 떨어진 곳에 존재함을 시사하는 동시적 주기 편차를 보입니다. 가시광 대응체나...
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이미지 전체보기 (30개)
![[PDF] First high-resolution radio study of the supernova remnant G338.3-0.0 associated with the gamma-ray source HESS J1640-465...](https://search.pstatic.net/sunny/?type=b150&src=https://figures.semanticscholar.org/286ff707a767290b956407f2c91fbb0bb8c7c940/6-Figure4-1.png)
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![[PDF] First high-resolution radio study of the supernova remnant G338.3-0.0 associated with the gamma-ray source HESS J1640-465...](https://search.pstatic.net/sunny/?type=b150&src=https://figures.semanticscholar.org/286ff707a767290b956407f2c91fbb0bb8c7c940/5-Figure3-1.png)
![[PDF] Reconciling Optical and Radio Observations of the Binary Millisecond Pulsar PSR J1640+2224 | Semantic Scholar](https://search.pstatic.net/sunny/?type=b150&src=https://d3i71xaburhd42.cloudfront.net/a12200da325ec16273bcb837971702466980720d/4-Figure4-1.png)
![[PDF] Reconciling Optical and Radio Observations of the Binary Millisecond Pulsar PSR J1640+2224 | Semantic Scholar](https://search.pstatic.net/sunny/?type=b150&src=https://d3i71xaburhd42.cloudfront.net/a12200da325ec16273bcb837971702466980720d/4-Figure3-1.png)
![[PDF] HESS J1640-465 - an exceptionally luminous TeV gamma-ray supernova remnant | Semantic Scholar](https://search.pstatic.net/sunny/?type=b150&src=https://figures.semanticscholar.org/48b57165a3e97ed1b7210ecafddeca661bd5f195/3-Figure1-1.png)
![[PDF] HESS J1640-465 - an exceptionally luminous TeV gamma-ray supernova remnant | Semantic Scholar](https://search.pstatic.net/sunny/?type=b150&src=https://figures.semanticscholar.org/48b57165a3e97ed1b7210ecafddeca661bd5f195/7-Figure4-1.png)
![[PDF] First high-resolution radio study of the supernova remnant G338.3-0.0 associated with the gamma-ray source HESS J1640-465...](https://search.pstatic.net/sunny/?type=b150&src=https://figures.semanticscholar.org/286ff707a767290b956407f2c91fbb0bb8c7c940/5-Figure2-1.png)
![[PDF] First high-resolution radio study of the supernova remnant G338.3-0.0 associated with the gamma-ray source HESS J1640-465...](https://search.pstatic.net/sunny/?type=b150&src=https://figures.semanticscholar.org/286ff707a767290b956407f2c91fbb0bb8c7c940/4-Figure1-1.png)
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