2007A&A...469..645S


C.D.S. - SIMBAD4 rel 1.7 - 2019.10.15CEST07:15:02

2007A&A...469..645S - Astronomy and Astrophysics, volume 469, 645-661 (2007/7-2)

SN2003du: 480 days in the life of a normal type Ia supernova.

STANISHEV V., GOOBAR A., BENETTI S., KOTAK R., PIGNATA G., NAVASARDYAN H., MAZZALI P., AMANULLAH R., GARAVINI G., NOBILI S., QIU Y., ELIAS-ROSA N., RUIZ-LAPUENTE P., MENDEZ J., MEIKLE P., PATAT F., PASTORELLO A., ALTAVILLA G., GUSTAFSSON M., HARUTYUNYAN A., IIJIMA T., JAKOBSSON P., KICHIZHIEVA M.V., LUNDQVIST P., MATTILA S., MELINDER J., PAVLENKO E.P., PAVLYUK N.N., SOLLERMAN J., TSVETKOV D.Y., TURATTO M. and HILLEBRANDT W.

Abstract (from CDS):

We present a study of the optical and near-infrared (NIR) properties of the Type Ia Supernova (SNIa) 2003du. An extensive set of optical and NIR photometry and low-resolution long-slit spectra was obtained using a number of facilities. The observations started 13 days before B-band maximum light and continued for 480 days with exceptionally good time sampling. The optical photometry was calibrated through the S-correction technique. The UBVRIJHK light curves and the color indices of SN2003du closely resemble those of normal SNeIa. SN2003du reached a B-band maximum of 13.49±0.02mag on JD2452766.38±0.5. We derive a B-band stretch parameter of 0.988±0.003, which corresponds to Δm15=1.02±0.05, indicative of a SNIa of standard luminosity. The reddening in the host galaxy was estimated by three methods, and was consistently found to be negligible. Using an updated calibration of the V and JHK absolute magnitudes of SNeIa, we find a distance modulus µ=32.79±0.15 mag to the host galaxy, UGC 9391. We measure a peak uvoir bolometric luminosity of 1.35(±0.20)x1043erg/s and Arnett's rule implies that M56^Ni≃0.68±0.14M☉_ of [][56]Ni was synthesized during the explosion. Modeling of the uvoir bolometric light curve also indicates M56^Ni_ in the range 0.6-0.8M. The spectral evolution of SN2003du at both optical and NIR wavelengths also closely resembles normal SNeIa. In particular, the SiII ratio at maximum R(SiII)=0.22±0.02 and the time evolution of the blueshift velocities of the absorption line minima are typical. The pre-maximum spectra of SN2003du showed conspicuous high-velocity features in the CaII H&K doublet and infrared triplet, and possibly in SiIIλ6355, lines. We compare the time evolution of the profiles of these lines with other well-observed SNeIa and we suggest that the peculiar pre-maximum evolution of SiIIλ6355 line in many SNeIa is due to the presence of two blended absorption components.

Abstract Copyright:

Journal keyword(s): stars: supernovae: general - stars: supernovae: individual: SN 2003du - methods: observational - techniques: photometric - techniques: spectroscopic

Nomenclature: Fig.1, Table 2: [SGB2007] NN (Nos 1-12).

CDS comments: Par. 3 : star AS 24 = [HMT98] AS 24-0

Simbad objects: 30

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Number of rows : 30

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2019
#notes
1 SN 2000cx SN* 01 24 46.19 +09 30 31.3   13.3       SN.Iap 192 1
2 SN 2004dt SN* 02 02 12.342 -00 06 02.10   15.33       SNIa 112 1
3 SN 1992A SN* 03 36 27.41 -34 57 31.4   12.56 12.50     SNIa 378 1
4 SN 2001el SN* 03 44 30.60 -44 38 23.4   12.81       SN.Ia 236 1
5 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 14317 1
6 SN 2004S SN* 06 45 43.50 -31 13 52.5   14.14 14.39     SN.Ia 61 1
7 SN 2003cg SN* 10 14 15.97 +03 28 02.5   15.94       SN.Ia 120 1
8 SN 2002bo SN* 10 18 06.51 +21 49 41.7   13.95       SN.Ia 264 1
9 SN 1998bu SN* 10 46 46.01 +11 50 07.5   12.11       SN.Ia 290 1
10 SN 1994ae SN* 10 47 01.94 +17 16 30.8   13.20 12.99     SNIa 148 1
11 SN 2006cf SN* 10 54 02.58 +46 01 36.3     18     SNIa 29 1
12 SN 1989B SN* 11 20 13.93 +13 00 18.9   12.25       SNIa 336 1
13 SN 1998aq SN* 11 56 25.87 +55 07 43.2   12.31 14.9     SNIa 165 1
14 SN 1994D SN* 12 34 02.395 +07 42 05.70   11.75 12.03     SNIa 519 1
15 SN 1981B SN* 12 34 29.57 +02 11 59.3   11.74       SNIa 381 1
16 HD 109596 PM* 12 35 15.3512319189 +62 56 56.985180021   9.83 9.68     A5V 5 0
17 SN 1990N SN* 12 42 56.68 +13 15 23.4   12.69 12.62     SNIa 368 1
18 SN 2002dj SN* 13 13 00.34 -19 31 08.7     17.0     SN.Ia 93 1
19 SN 1996X SN* 13 18 01.13 -26 50 45.3   12.99 13.00     SNIa 173 1
20 SN 2000ca SN* 13 35 22.98 -34 09 37.0   15.90       SN.Ia 47 2
21 SN 2003du SN* 14 34 35.80 +59 20 03.8   13.46       SN.Ia 305 1
22 UGC 9391 G 14 34 37.013 +59 20 16.17   15.5       ~ 68 0
23 HD 132254 PM* 14 56 23.0406690689 +49 37 42.416350556   6.13   5.3   F8-V 116 0
24 SN 2005cf SN* 15 21 33.12 -07 26 57.1   13.54       SN.Ia 226 1
25 SN 2002er SN* 17 11 29.88 +07 59 44.8   14.25       SNIa 114 1
26 M 92 GlC 17 17 07.39 +43 08 09.4     6.52     ~ 1864 0
27 SN 2004eo SN* 20 32 54.19 +09 55 42.7   15.07 17.8     SN.Ia 159 1
28 SN 2005cg SN* 21 10 50.44 +00 12 06.8     18.2     SNIa 31 1
29 SN 1999ee SN* 22 16 09.40 -36 50 31.5   14.85       SN.Ia 169 1
30 NAME Local Group GrG ~ ~           ~ 6652 0

    Equat.    Gal    SGal    Ecl

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2019.10.15-07:15:02

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