粗鄙的人 发表于 2025-3-30 11:58:14

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certitude 发表于 2025-3-30 15:42:38

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gospel 发表于 2025-3-30 19:01:22

Supernova of 1006 (G327.6+14.6)on. Therefore, most of iron might have escaped from the ultraviolet background sources. Another important aspect with SN 1006 is that it was the first SNR in which synchrotron X-ray emission was detected from shells of the remnant, providing evidence that electrons are accelerated up to ∼ 100 TeV en

sacrum 发表于 2025-3-30 23:11:42

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Tremor 发表于 2025-3-31 02:45:45

Supernova 1604, Kepler’s Supernova, and its Remnantrf and an evolved companion star, which most likely was in the (post)-asymptotic giant branch of its evolution. A problem with this scenario is that the companion star must have survived the explosion, but no trace of its existence has yet been found, despite a deep search.

PANT 发表于 2025-3-31 08:37:11

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查看完整版本: Titlebook: Handbook of Supernovae; Athem W. Alsabti,Paul Murdin Reference work 2017 Springer International Publishing AG 2017 Cosmology from Supernov