Anomalous extinction behaviour towards the type Ia SN 2003cg

被引:131
作者
Elias-Rosa, N.
Benetti, S.
Cappellaro, E.
Turatto, M.
Mazzali, P. A.
Patat, F.
Meikle, W. P. S.
Stehle, M.
Pastorello, A.
Pignata, G.
Kotak, R.
Harutyunyan, A.
Altavilla, G.
Navasardyan, H.
Qiu, Y.
Salvo, M.
Hillebrandt, W.
机构
[1] Astron Observ Padova, INAF, I-35122 Padua, Italy
[2] Univ La Laguna, E-38206 Tenerife, Spain
[3] Max Planck Inst Astrophys, D-85748 Garching, Germany
[4] Osserv Astron Trieste, INAF, I-34131 Trieste, Italy
[5] European So Observ, D-85748 Garching, Germany
[6] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England
[7] Pontifica Univ Catolica, Dept Astron & Astrofis, Santiago, Chile
[8] Univ Barcelona, Dept Astron & Meteorol, E-08028 Barcelona, Spain
[9] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
[10] Australian Natl Univ, Mt Stromlo Observ, Weston, ACT 2611, Australia
关键词
supernovae : general; supernovae : individual : SN 2003cg; dust; extinction;
D O I
10.1111/j.1365-2966.2006.10430.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present optical and near-infrared photometry and spectroscopy of the Type Ia SN 2003cg, which exploded in the nearby galaxy NGC 3169. The observations cover a period between -8.5 and +414 d post-maximum. SN 2003cg is a normal but highly reddened Type Ia event. Its B magnitude at maximum B-max = 15.94 +/- 0.04 and Delta m(15)(B)(obs) = 1.12 +/- 0.04 [Delta m(15)(B)(intrinsic) = 1.25 +/- 0.05]. Allowing R-V to become a free parameter within the Cardelli et al. extinction law, simultaneous matches to a range of colour curves of normal SNe Ia yielded E(B - V) = 1.33 +/- 0.11, and RV = 1.80 +/- 0.19. While the value obtained for R-V is small, such values have been invoked in the past, and may imply a grain size which is small compared with the average value for the local interstellar medium.
引用
收藏
页码:1880 / 1900
页数:21
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