NAOC Open IR
radiospectraofthreesupernovaremnantsg114303g116511andg116902
Wenwu Tian1; Denis Leahy2
2006
Source Publicationchinesejournalofastronomyandastrophysics
ISSN1009-9271
Volume6Issue:5Pages:543
AbstractPresented are new images of supernova. remnants G114.3+0.3, G116.5+1.1 and G116.9+0.2 (CTB 1) at 408 MHz from the Canadian Galactic Plane Survey (CGPS). We also use the 1420 MHz images from the CGPS in a study of their 408-1420 MHz spectral indices. The flux densities at 408 MHz and 1420 MHz, corrected for flux densities from compact sources within the SNRs, are 12 +/- 6 Jy and 9.8 +/- 0.8 Jy for G114.3+0.3, 15.0 +/- 1.5 Jy and 10.6 +/- 0.6 Jy for G116.5+1.1, 15.0+/-1.5 Jy and 8.1 +/- 0.4 Jy for G116.9+0.2. The integrated flux density-based spectral indices (S-nu proportional to nu(-alpha)) are alpha=0.16 +/- 0.41, 0.28 +/- 0.09 and 0.49 +/- 0.09 for G114.3+0.3, G116.5+1.1 and. G116.9+0.2, respectively. Their T-T plot-based spectral indices are 0.68 +/- 0.48, 0.28 +/- 0.15, and 0.48 +/- 0.04, in agreement with the integrated flux density-based spectral indices. New flux densities are derived at 2695 MHz which are significantly larger than previous values. The new 408, 1420 and 2695 MHz flux densities and published values at other frequencies, where images are not available, are fitted After correcting for contributions from compact sources, to derive their multi-frequency spectral indices.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/51581
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.卡尔加里大学
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Wenwu Tian,Denis Leahy. radiospectraofthreesupernovaremnantsg114303g116511andg116902[J]. chinesejournalofastronomyandastrophysics,2006,6(5):543.
APA Wenwu Tian,&Denis Leahy.(2006).radiospectraofthreesupernovaremnantsg114303g116511andg116902.chinesejournalofastronomyandastrophysics,6(5),543.
MLA Wenwu Tian,et al."radiospectraofthreesupernovaremnantsg114303g116511andg116902".chinesejournalofastronomyandastrophysics 6.5(2006):543.
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