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An optical supernova associated with the X-ray flash XRF 060218
Pian, E.; Mazzali, P. A.; Masetti, N.; Ferrero, P.; Klose, S.; Palazzi, E.; Ramirez-Ruiz, E.; Woosley, S. E.; Kouveliotou, C.; Deng, J.; Filippenko, A. V.; Foley, R. J.; Fynbo, J. P. U.; Kann, D. A.; Li, W.; Hjorth, J.; Nomoto, K.; Patat, F.; Sauer, D. N.; Sollerman, J.; Vreeswijk, P. M.; Guenther, E. W.; Levan, A.; O'Brien, P.; Tanvir, N. R.; Wijers, R. A. M. J.; Dumas, C.; Hainaut, O.; Wong, D. S.; Baade, D.; Wang, L.; Amati, L.; Cappellaro, E.; Castro-Tirado, A. J.; Ellison, S.; Frontera, F.; Fruchter, A. S.; Greiner, J.; Kawabata, K.; Ledoux, C.; Maeda, K.; Moller, P.; Nicastro, L.; Rol, E.; Starling, R.
2006-08-31
Source PublicationNATURE
ISSN0028-0836
Volume442Issue:7106Pages:1011-1013
AbstractLong-duration gamma-ray bursts (GRBs) are associated with type Ic supernovae(1) that are more luminous than average(2-5) and that eject material at very high velocities. Less-luminous supernovae were not hitherto known to be associated with GRBs, and therefore GRB - supernovae were thought to be rare events(6). Whether X-ray flashes - analogues of GRBs, but with lower luminosities and fewer gamma-rays - can also be associated with supernovae, and whether they are intrinsically 'weak' events or typical GRBs viewed off the axis of the burst(7), is unclear. Here we report the optical discovery and follow-up observations of the type Ic supernova SN 2006aj associated with X-ray flash XRF 060218. Supernova 2006aj is intrinsically less luminous than the GRB - supernovae, but more luminous than many supernovae not accompanied by a GRB. The ejecta velocities derived from our spectra are intermediate between these two groups, which is consistent with the weakness of both the GRB output(8) and the supernova radio flux(9). Our data, combined with radio and X-ray observations(8-10), suggest that XRF 060218 is an intrinsically weak and soft event, rather than a classical GRB observed off-axis. This extends the GRB - supernova connection to X-ray flashes and fainter supernovae, implying a common origin. Events such as XRF 060218 are probably more numerous than GRB - supernovae.
KeywordLow-luminosity Light-curve Burst Afterglow Models Grb-030329 Grb-031203 Discovery Sn-2006aj Emission
Subject AreaScience & Technology - Other Topics
WOS HeadingsScience & Technology
DOI10.1038/nature05082
WOS KeywordLOW-LUMINOSITY ; LIGHT-CURVE ; BURST ; AFTERGLOW ; MODELS ; GRB-030329 ; GRB-031203 ; DISCOVERY ; SN-2006AJ ; EMISSION
Indexed BySCI
Language英语
WOS Research AreaScience & Technology - Other Topics
WOS SubjectMultidisciplinary Sciences
WOS IDWOS:000240142000042
Citation statistics
Cited Times:383[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/3640
Collection期刊(老文献)
Affiliation1.Trieste Astron Observ, Ist Nazl Astrofis, I-34131 Trieste, Italy
2.Univ Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA
3.Max Planck Inst Astrophys, D-85748 Garching, Germany
4.Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan
5.Univ Tokyo, Sch Sci, Res Ctr Early Universe, Bunkyo Ku, Tokyo 1130033, Japan
6.IASF, Ist Nazl Astrofis, I-40129 Bologna, Italy
7.Thuringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany
8.Inst Adv Study, Princeton, NJ 08540 USA
9.Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA
10.NASA, MSFC, NSSTC, Huntsville, AL 35805 USA
11.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
12.Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
13.Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, DK-2100 Copenhagen O, Denmark
14.European So Observ, D-85748 Garching, Germany
15.Stockholm Univ, Dept Astron, S-10691 Stockholm, Sweden
16.Univ Chile, Dept Astron, Santiago, Chile
17.European So Observ, Santiago 19, Chile
18.Univ Hertfordshire, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England
19.Univ Leicester, Dept Phys & Astron, Xray & Observat Astron Grp, Leicester LE1 7RH, Leics, England
20.Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
21.Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA
22.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
23.Padova Astron Observ, Ist Nazl Astrofis, I-35122 Padua, Italy
24.CSIC, IAA, E-18080 Granada, Spain
25.Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 1A1, Canada
26.Univ Ferrara, Dept Phys, I-44100 Ferrara, Italy
27.Space Telescope Sci Inst, Baltimore, MD 21218 USA
28.Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
29.Hiroshima Univ, Hiroshima Astrophys Sci Ctr, Hiroshima 7398526, Japan
30.Univ Tokyo, Coll Arts & Sci, Dept Earth Sci & Astron, Meguro Ku, Tokyo 1538902, Japan
Recommended Citation
GB/T 7714
Pian, E.,Mazzali, P. A.,Masetti, N.,et al. An optical supernova associated with the X-ray flash XRF 060218[J]. NATURE,2006,442(7106):1011-1013.
APA Pian, E..,Mazzali, P. A..,Masetti, N..,Ferrero, P..,Klose, S..,...&Starling, R..(2006).An optical supernova associated with the X-ray flash XRF 060218.NATURE,442(7106),1011-1013.
MLA Pian, E.,et al."An optical supernova associated with the X-ray flash XRF 060218".NATURE 442.7106(2006):1011-1013.
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