insert
发表于 2025-3-23 10:20:20
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木讷
发表于 2025-3-23 17:21:15
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本土
发表于 2025-3-23 21:41:43
Conservation and Efficiency Issues, to 2002 and show our result on moderately to strongly decelerated expansion with . = 0.71 ± 0.11. We comment on our result of an inversion of the radio spectrum in terms of the emergence of a possible pulsar nebula.
subordinate
发表于 2025-3-23 22:41:37
Conservation and Efficiency Issues,ount of relativistic ejecta, it produces a radio luminosity which is comparable to that seen in the unusual SN1998bw. Using SN2003L as an example, we comment briefly on the broad diversity of type Ic properties and the associated implications for progenitor models.
GRAZE
发表于 2025-3-24 02:30:22
A Decade of Radio and X-ray Observations of SN 1993Je fully-developed dataset, and compare this to our earlier characterization made in 1994. SN 1993J has also been a target of X-ray satellites, and we briefly discuss the nature of the X-ray emission and, together with the radio emission, describe the implications for the nature of the SN’s progenitor.
SKIFF
发表于 2025-3-24 09:04:06
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Interlocking
发表于 2025-3-24 11:16:32
Optical, Ultraviolet, and Infrared Observations of SN 1993Jmission comes from the collision of supernova ejecta with circumstellar gas that was released by the progenitor prior to the explosion. The circumstellar material shows strong evidence of CNO processing.
VEST
发表于 2025-3-24 15:36:24
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贝雷帽
发表于 2025-3-24 21:04:02
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摊位
发表于 2025-3-25 02:30:19
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