2020MNRAS.499..974G


Query : 2020MNRAS.499..974G

2020MNRAS.499..974G - Mon. Not. R. Astron. Soc., 499, 974-992 (2020/November-3)

SN 2017ivv: two years of evolution of a transitional Type II supernova.

GUTIERREZ C.P., PASTORELLO A., JERKSTRAND A., GALBANY L., SULLIVAN M., ANDERSON J.P., TAUBENBERGER S., KUNCARAYAKTI H., GONZALEZ-GAITAN S., WISEMAN P., INSERRA C., FRASER M., MAGUIRE K., SMARTT S., MULLER-BRAVO T.E., ARCAVI I., BENETTI S., BERSIER D., BOSE S., BOSTROEM K.A., BURKE J., CHEN P., CHEN T.-W., DELLA VALLE M., DONG S., GAL-YAM A., GROMADZKI M., HIRAMATSU D., HOLOIEN T.W.-S., HOSSEINZADEH G., HOWELL D.A., KANKARE E., KOCHANEK C.S., McCULLY C., NICHOLL M., PIGNATA G., PRIETO J.L., SHAPPEE B., TAGGART K., TOMASELLA L., VALENTI S. and YOUNG D.R.

Abstract (from CDS):

We present the photometric and spectroscopic evolution of the Type II supernova (SN II) SN 2017ivv (also known as ASASSN-17qp). Located in an extremely faint galaxy (Mr = -10.3 mag), SN 2017ivv shows an unprecedented evolution during the 2 yr of observations. At early times, the light curve shows a fast rise (∼6-8 d) to a peak of M^ max^g= -17.84 mag, followed by a very rapid decline of 7.94 ± 0.48 mag per 100 d in the V band. The extensive photometric coverage at late phases shows that the radioactive tail has two slopes, one steeper than that expected from the decay of 56Co (between 100 and 350 d), and another slower (after 450 d), probably produced by an additional energy source. From the bolometric light curve, we estimated that the amount of ejected 56Ni is ∼0.059 ± 0.003 M☉. The nebular spectra of SN 2017ivv show a remarkable transformation that allows the evolution to be split into three phases: (1) Hα strong phase (<200 d); (2) Hα weak phase (between 200 and 350 d); and (3) Hα broad phase (>500 d). We find that the nebular analysis favours a binary progenitor and an asymmetric explosion. Finally, comparing the nebular spectra of SN 2017ivv to models suggests a progenitor with a zero-age main-sequence mass of 15-17 M.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): techniques: photometric - techniques: spectroscopic - surveys - supernovae: general

Simbad objects: 41

goto Full paper

goto View the references in ADS

Number of rows : 41
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 SN 2004fe SN* 00 30 11.27 +02 05 23.5     18.1     SNIc 45 1
2 SN 2016gkg SN* 01 34 14.46 -29 26 25.0           SNIIb 77 0
3 SN 2002ap SN* 01 36 23.85 +15 45 13.2   13.11 14.54     SNIc-BL 547 1
4 SN 2013ej SN* 01 36 48.16 +15 45 31.0           SNIIP 173 0
5 SN 2011fu SN* 02 08 21.40 +41 29 12.3           SNII 47 1
6 SN 1997D SN* 04 11 01.00 -56 29 56.0       16.3   SNIIpec 171 1
7 SN 1999em SN* 04 41 27.04 -02 51 45.2   13.79 13.7     SNIIP 648 1
8 SN 2004gq SN* 05 12 04.81 -15 40 54.2     15.5     SNIb 88 1
9 SN 1987A SN* 05 35 28.020 -69 16 11.07           SNIIpec 4784 2
10 SN 1995ad SN* 06 01 06.13 -23 40 29.0       15.7   SNII 48 1
11 SN 1993J SN* 09 55 24.77476 +69 01 13.7026   10.8 12.0     SNIIb 1364 1
12 SN 2015as SN* 10 08 11.37 +51 50 40.9           SNII 7 1
13 SN 2005bf SN* 10 23 56.99 -03 11 29.3     18.0     SNIb 191 1
14 SN 2012aw SN* 10 43 53.735 +11 40 17.63       15   SNIIP 179 1
15 SN 2014G SN* 10 54 34.13 +54 17 56.9           SNIIL 49 1
16 SN 1996cb SN* 11 03 41.98 +28 54 13.7   14.22       SNIIb 106 1
17 SN 1998A SN* 11 09 50.33 -23 43 43.1       17.0   SNIIpec 51 1
18 SN 2006bp SN* 11 53 55.74 +52 21 09.4 14.5 15.8 14.7     SNIIP 169 1
19 SN 2004gk SN* 12 25 33.21 +12 15 39.9     13.3     SNIc 36 1
20 SN 2013df SN* 12 26 29.33 +31 13 38.3           SNIIb 98 1
21 SN 2008ax SN* 12 30 40.80 +41 38 16.1   23.6 23.5 14.1 22.6 SNIIb 245 1
22 SN 1987K SN* 12 43 41.17 +16 23 44.9     14.2     SNIIb: 145 1
23 SN 2011dh SN* 13 30 05.10555 +47 10 10.9227           SNIIb 353 1
24 SN 1992H SN* 13 56 22.26 +47 14 27.4     15.0     SNII 104 1
25 SN 1996aq SN* 14 22 22.72 -00 23 23.8     15.7     SNIc 44 1
26 SN 2007X SN* 14 30 14.50 -36 57 53.1     15.3     SNII 16 1
27 SN 2013dh SN* 15 30 01.0 +12 59 21           SNIapec 14 1
28 SN 2010as SN* 15 49 49.23 -29 23 09.7           SNIb/c 27 1
29 SN 2013by SN* 16 59 02.43 -60 11 41.8           SNII 55 1
30 SN 2016esw SN* 18 58 04.090 +43 56 22.60           SNII 12 0
31 ASASSN -15oz SN* 19 19 33.49 -33 46 02.0           SNII 15 0
32 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1764 2
33 GALEXASC J202849.46-042255.5 G 20 28 49.46 -04 22 55.5           ~ 1 0
34 SN 2017ivv SN* 20 28 49.800 -04 22 57.29           SNII 9 0
35 SN 2004et SN* 20 35 25.33 +60 07 17.7   12.88       SNIIP 464 1
36 SN 1980K SN* 20 35 30.07 +60 06 23.7   11.6       SNIIL 453 1
37 SN 2015bs SN* 22 33 43.78 -06 22 08.1           SNII 14 0
38 SN 2011hs SN* 22 57 11.77 -43 23 04.8           SNIIb 44 1
39 SN 2009jf SN* 23 04 52.98 +12 19 59.5           SNIb 99 1
40 SN 2003jd SN* 23 21 03.38 -04 53 45.5   16.34       SNIc-BL 137 1
41 SN 2007od SN* 23 55 48.68 +18 24 54.8       14.4   SNIIP 123 1

To bookmark this query, right click on this link: simbad:objects in 2020MNRAS.499..974G and select 'bookmark this link' or equivalent in the popup menu


2023.02.07-18:53:01

© Université de Strasbourg/CNRS

    • Contact