单色
发表于 2025-3-23 13:33:44
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intention
发表于 2025-3-23 14:11:31
Conference proceedings 1988plosions and deeper understanding of the experimental data. Properties of supernova shells are discussed, such as their kinematics, ages, sizes, temperatures, spectra, polarizations, energetics and morphologies. Special attention is given to a few shells of extreme age, viz. G 70.68+1.20, Kepler‘s SN, and CTB 80, as well as to their statistics.
Junction
发表于 2025-3-23 21:19:12
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frugal
发表于 2025-3-24 00:51:19
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ALB
发表于 2025-3-24 06:04:51
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圆桶
发表于 2025-3-24 09:14:09
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Systemic
发表于 2025-3-24 14:29:19
,G316.3-0.0 and G332A+0.1 — Two supernova remnants with blowouts,High-resolution 843 MHz observations of the supernova remnants G316.3-0.0 and G332.4+0.1 exhibit forms which suggest that the spherical shells have blown out over part of their surface into adjacent lower-density regions. This view is reinforced by observations of the polarization, and hence the magnetic field directions, in these objects.
载货清单
发表于 2025-3-24 17:31:50
High resolution radio observations of G11.2-0.3,High-resolution (3 arcsec) radio observations of the relatively bright `shell‘ SNR G11.2-0.3 made with the VLA at 1.46 and 4.76 GHz are presented. These reveal a clumpy shell of emission, which resembles an evolved version of Cassiopeia A, rather than the smooth shell of emission that is seen from the remnants of Tycho‘s and Kepler‘s SN.
forbid
发表于 2025-3-24 19:43:22
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积习难改
发表于 2025-3-24 23:19:55
Lecture Notes in Physicshttp://image.papertrans.cn/t/image/881889.jpg