Keck and European southern observatory very large telescope view of the symmetry of the ejecta of the XRF/SN 2006aj
文献类型：期刊论文
| 作者 | Mazzali, Paolo A.; Foley, Ryan J.; Deng, Jinsong; Patat, Ferdinando; Pian, Elena; Baade, Dietrich; Bloom, Joshua S.; Filippenko, Alexei V.; Perley, Daniel A.; Valenti, Stefano |
| 刊名 | ASTROPHYSICAL JOURNAL
 |
| 出版日期 | 2007-06-01 |
| 卷号 | 661期号:2页码:892-898 |
| 关键词 | gamma rays : bursts nuclear reactions, nucleosynthesis, abundances supernovae : general supernovae : individual (SN 2006aj) |
| 英文摘要 | Nebular-phase spectra of SN 2006aj, discovered in coincidence with XRF 060218, were obtained with Keck in 2006 July and VLT in 2006 September. At the latter epoch spectropolarimetry was also attempted, yielding a polarization upper limit of similar to 2%. The spectra show strong [O I] and Mg I] emission lines, as expected in Type Ic supernovae, but weak Ca ii lines. The [ Fe ii] lines that were strong in SN 1998bw are much weaker in SN 2006aj, consistent with its lower luminosity. The outer velocity of the line-emitting region is similar to 8000 km s(-1) in July and similar to 7400 km s(-1) in September, consistent with the relatively low expansion kinetic energy of SN 2006aj. All lines have similar width, and their profiles indicate that no major asymmetries are present in the ejecta at velocities below v < 8000 km s(-1), except perhaps in the innermost part. The spectra were modeled with a non-LTE code. The mass of (56)Ni required to power the emission is similar to 0: 20 M(circle dot), confirming earlier results based on the light curve. The oxygen mass is similar to 1: 5 M(circle dot), again much less than in SN 1998bw, but similar to 0: 7 M(circle dot) larger than the value derived from the early-time modeling. The ejected mass below 8000 km s(-1) is similar to 2 M(circle dot), confirming that SN 2006aj was only about twice as massive and energetic as the normal Type Ic SN 1994I. The presence of a dense inner core, containing similar to 1 M(circle dot) of mostly oxygen and carbon, is inferred, as in all broad-lined SNe Ic. This core, which may be disklike, is too deep to influence the early light curve and too small to affect the late polarization spectrum. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | GAMMA-RAY BURST ; IC HYPERNOVA SN-2003DH/GRB-030329 ; LATE-TIME SPECTRA ; 25 APRIL 1998 ; SN 1998BW ; OFF-AXIS ; NEBULAR SPECTRA ; SUPERNOVA 2002AP ; CORE-COLLAPSE ; LIGHT CURVES |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000246947100022 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/15873]  |
| 专题 | 紫金山天文台_南极天文中心 |
| 作者单位 | 1.Max Planck Inst Astrophys, D-85748 Garching, Germany 2.Natl Inst Astrophys, OATs, I-34143 Trieste, Italy 3.Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan 4.Univ Tokyo, Sch Sci, Res Ctr Early Universe, Bunkyo Ku, Tokyo 1130033, Japan 5.Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA 6.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 7.European So Observ, D-85748 Garching, Germany 8.Univ Ferrara, Dept Phys, I-44100 Ferrara, Italy 9.Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA 10.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China |
| 推荐引用方式 GB/T 7714 | Mazzali, Paolo A.,Foley, Ryan J.,Deng, Jinsong,et al. Keck and European southern observatory very large telescope view of the symmetry of the ejecta of the XRF/SN 2006aj[J]. ASTROPHYSICAL JOURNAL,2007,661(2):892-898. |
| APA | Mazzali, Paolo A..,Foley, Ryan J..,Deng, Jinsong.,Patat, Ferdinando.,Pian, Elena.,...&Nomoto, Ken-Ichi.(2007).Keck and European southern observatory very large telescope view of the symmetry of the ejecta of the XRF/SN 2006aj.ASTROPHYSICAL JOURNAL,661(2),892-898. |
| MLA | Mazzali, Paolo A.,et al."Keck and European southern observatory very large telescope view of the symmetry of the ejecta of the XRF/SN 2006aj".ASTROPHYSICAL JOURNAL 661.2(2007):892-898. |
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来源：紫金山天文台
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