SN 2005at-A neglected type Ic supernova at 10 Mpc

被引:17
作者
Kankare, E. [1 ,2 ]
Fraser, M. [3 ]
Ryder, S. [4 ]
Romero-Canizales, C. [5 ,6 ]
Mattila, S. [2 ]
Kotak, R. [7 ]
Laursen, P. [8 ]
Monard, L. A. G. [9 ]
Salvo, M. [10 ]
Vaeisaenen, P. [11 ,12 ]
机构
[1] Univ Turku, Dept Phys & Astron, Tuorla Observ, Piikkio 21500, Finland
[2] Univ Turku, Finnish Ctr Astron ESO FINCA, Piikkio 21500, Finland
[3] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[4] Australian Astron Observ, N Ryde, NSW 1670, Australia
[5] Pontificia Univ Catolica Chile, Fac Fis, Inst Astrofis, Santiago 22, Chile
[6] Millennium Inst Astrophys, Santiago, Chile
[7] Queens Univ Belfast, Sch Math & Phys, Astrophys Res Ctr, Belfast BT7 1NN, Antrim, North Ireland
[8] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, DK-2100 Copenhagen, Denmark
[9] Ctr Backyard Astrophys Pretoria, Bronberg Observ, ZA-0056 Tiegerpoort, South Africa
[10] Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia
[11] S African Astron Observ, ZA-7935 Cape Town, South Africa
[12] Southern African Large Telescope, ZA-7935 Cape Town, South Africa
基金
芬兰科学院;
关键词
supernovae: general; supernovae: individual: SN 2005at; supernovae: individual: SN 2007gr; CORE-COLLAPSE SUPERNOVAE; SPITZER-SPACE-TELESCOPE; EXTRAGALACTIC DISTANCE DATABASE; STAR-FORMATION RATE; X-RAY OBSERVATIONS; CIRCUMSTELLAR MEDIUM; IMAGE SUBTRACTION; BINARY PROGENITOR; INFRARED ECHO; IIP SUPERNOVA;
D O I
10.1051/0004-6361/201424563
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a photometric and spectroscopic study of a reddened type Ic supernova (SN) 2005at. We report our results based on the available data of SN 2005at, including late-time observations from the Spitzer Space Telescope and the Hubble Space Telescope. In particular, late-time mid-infrared observations are something rare for type Ib/c SNe. In our study we find SN 2005at to be very similar photometrically and spectroscopically to another nearby type Ic SN 2007gr, underlining the prototypical nature of this well-followed type Ic event. The spectroscopy of both events shows similar narrow spectral line features. The radio observations of SN 2005at are consistent with fast evolution and low luminosity at radio wavelengths. The late-time Spitzer data suggest the presence of an unresolved light echo from interstellar dust and dust formation in the ejecta, both of which are unique observations for a type Ic SN. The late-time Hubble observations reveal a faint point source coincident with SN 2005at, which is very likely either a declining light echo of the SN or a compact cluster. For completeness we study ground-based pre-explosion archival images of the explosion site of SN 2005at, however this only yielded very shallow upper limits for the SN progenitor star. We derive a host galaxy extinction of AV approximate to 1.9 mag for SN 2005at, which is relatively high for a SN in a normal spiral galaxy not viewed edge-on.
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页数:13
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