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Imprints of the Jittering Jets Explosion Mechanism in the Morphology of the Supernova Remnant SNR 0540-69.3
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作者 Noam Soker 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2022年第3期186-193,共8页
I identify a point-symmetric structure in recently published VLT/MUSE velocity maps of different elements in a plane along the line of sight at the center of the supernova remnant SNR 0540-69.3,and argue that jitterin... I identify a point-symmetric structure in recently published VLT/MUSE velocity maps of different elements in a plane along the line of sight at the center of the supernova remnant SNR 0540-69.3,and argue that jittering jets that exploded this core collapse supernova shaped this point-symmetric structure.The four pairs of two opposite clumps that compose this point symmetric structure suggest that two to four pairs of jittering jets shaped the inner ejecta in this plane.In addition,intensity images of several spectral lines reveal a faint strip(the main jet-axis)that is part of this plane of jittering jets and its similarity to morphological features in a few other SNRs and in some planetary nebulae further suggests shaping by jets.My interpretation implies that in addition to instabilities,jets also mix elements in the ejecta of core collapse supernovae.Based on the point-symmetric structure and under the assumption that jittering jets exploded this supernova,I estimate the component of the neutron star natal kick velocity on the plane of the sky to be■235 km s^(-1),and at an angle of■47°to the direction of the main jet-axis.I analyze this natal kick direction together with 12 other SNRs in the frame of the jittering jets explosion mechanism. 展开更多
关键词 ISM:supernova remnants stars:jets (stars:)supernovae:general (stars:)supernovae:individual(snr 0540-69.3)
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太阳附近恒星的空间分布
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作者 应晓 侯金良 傅承启 《中国科学院上海天文台年刊》 1998年第19期113-118,共6页
以近距星星表第兰版(CNS3)为样本,统计了太阳附近恒星的空间分布情况,结果发现在太阳附近恒星分布十分不均匀,许多地方密度极小,甚至为零,我们称其为空洞。本文给出了这些空洞的位置和大小,并提出它们可能与超新星爆发有关。
关键词 太阳系起源 太阳系演化 超新星遗迹 恒星 空间分布 空洞
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