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FUV Spectral Images of the Vela Supernova Remnant: Comparisons with X-ray and $H{alpha}$ images
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  • FUV Spectral Images of the Vela Supernova Remnant: Comparisons with X-ray and $H{alpha}$ images
  • FUV Spectral Images of the Vela Supernova Remnant: Comparisons with X-ray and $H{alpha}$ images
저자명
김일중,선광일,민경욱,한원용,Kim. Il-Joong,Seon. Kwang-Il,Min. Kyoung-Wook,Han. Wonyong,Edelstein. Jerry
간행물명
천문학회보
권/호정보
2012년|37권 2호|pp.99-99 (1 pages)
발행정보
한국천문학회
파일정보
정기간행물|ENG|
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기타
이 논문은 한국과학기술정보연구원과 논문 연계를 통해 무료로 제공되는 원문입니다.
서지반출

기타언어초록

We updated the far-ultraviolet (FUV) spectral images of the entire Vela supernova remnant (SNR) using newly processed FIMS/SPEAR data. In the present study, we compare the newly produced FUV images with the X-ray and $H{alpha}$ images, and examine how the Vela SNR evolves and interacts with the ambient medium on a global scale. The comparison with X-ray images has revealed a FUV filamentary feature corresponding with the boundary of the northeast-southwest asymmetry of the X-ray shell. The relatively low O IV] ${lambda}1404$ to O III] ${lambda}{lambda}1661$, 1666 ratio estimated on the FUV filament is compatible with the previous proposal that the observed asymmetry of the Vela SNR could be due to the ${gamma}2$ Velorum stellar wind bubble (SWB). The southwest FUV features surrounding a faint extended X-ray region are characterized as the region where the Vela SNR is interacting slightly stronger with ambient mediums within the dim X-ray southwest section. From a comparison with the $H{alpha}$ image, we identify a ring-like $H{alpha}$ feature overlapped with an extended hot X-ray feature of similar size and two local peaks of C IV ${lambda}{lambda}1548$, 1551 emission. Their morphologies are consistent with the expected shape when the $H{alpha}$ ring is in direct contact with the near or far side of the Vela SNR. We suggest that the B3V-type star HD 76161 found at the center of the $H{alpha}$ ring would be the exciting source of the H II region.