Galactic Center Shells and a Recurrent Starburst Model
Galactic Center Shells and a Recurrent Starburst Model
复制标题
银河中心壳和循环星暴模型
DOI:
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发表时间:
2003
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影响因子:
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通讯作者:
Y. Sofue
中科院分区:
文献类型:
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作者:
Y. Sofue
By applying filtering techniques to remove straight filaments in the 20-cm VLA radio image of the Galactic Center Arc region, we have shown that numerous concentric radio shells of radii 5 to 20pc are surrounding the Pistol and Sickle region, which we call Galactic Center Shells (GCS). Each shell has thermal energy of the order of 10 49–50 erg. Several CO-line shells are associated, whose kinetic energies are of the order of 10 49–50 erg. Summing up the energies of recognized GCSs, the total energy amounts to ∼10 51 erg. The GCSs show an excellent correlation with the FIR shells observed at 16–26 µm with the MSX. We propose a model in which GCSs were produced by recurrent and/or intermittent starbursts in the Pistol area during the last million years. The most recent burst occurred some 10 5 years ago, producing an inner round-shaped shell (GCS I); earlier ones a million years ago produced outer shells (GCS II and III), which are more deformed by interactions with the surrounding ISM and Sgr A halo. We argue that recurrent starbursts had also occurred in the past, which produced larger scale hyper-shell structures as well. A burst some million years ago produced the Galactic Center Lobe, and a much stronger one 15 million years ago produced the North Polar Spur.