2007A&A...461..233U


C.D.S. - SIMBAD4 rel 1.7 - 2019.09.17CEST13:21:25

2007A&A...461..233U - Astronomy and Astrophysics, volume 461, 233-251 (2007/1-1)

An optimal hydrodynamic model for the normal type IIP supernova 1999em.

UTROBIN V.P.

Abstract (from CDS):

There is still no consensus about progenitor masses of type IIP supernovae. We study a normal type IIP SN 1999em in detail and compare it to a peculiar type IIP SN 1987A. We computed the hydrodynamic and time-dependent atmosphere models interpreting simultaneously both the photometric and spectroscopic observations. The bolometric light curve of SN 1999em and the spectral evolution of its Hα line are consistent with a presupernova radius of 500±200R, an ejecta mass of 19.0±1.2M, an explosion energy of (1.3±0.1)x1051erg, and a radioactive 56Ni mass of 0.036±0.009M. A mutual mixing of hydrogen-rich and helium-rich matter in the inner layers of the ejecta guarantees a good fit of the calculated light curve to that observed. Based on the hydrodynamic models in the vicinity of the optimal model, we derive the approximate relationships between the basic physical and observed parameters. The hydrodynamic and atmosphere models of SN 1999em are inconsistent with the short distance of 7.85Mpc to the host galaxy. We find that the hydrogen recombination in the atmosphere of a normal type IIP SN 1999em, as well as most likely other type IIP supernovae at the photospheric epoch, is essentially a time-dependent phenomenon. It is also shown that in normal type IIP supernovae the homologous expansion of the ejecta in its atmosphere takes place starting from nearly the third day after the supernova explosion. A comparison of SN 1999em with SN 1987A reveals two very important results for supernova theory. First, the comparability of the helium core masses and the explosion energies implies a unique explosion mechanism for these core collapse supernovae. Second, the optimal model for SN 1999em is characterized by a weaker 56Ni mixing up to ≃660km/s compared to a moderate 56Ni mixing up to ∼3000km/s in SN 1987A, hydrogen being mixed deeply downward to ∼650km/s.

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Journal keyword(s): stars: supernovae: individual: SN 1999em - stars: supernovae: individual: SN 1987A

Simbad objects: 9

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Number of rows : 9

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 1997D SN* 04 11 01.00 -56 29 56.0       16.3   SN.IIPec 155 1
2 SN 1999em SN* 04 41 27.04 -02 51 45.2   13.79 13.7     SN.IIP 552 1
3 NGC 1637 AGN 04 41 28.229 -02 51 28.94   11.4   11.0 11.3 ~ 365 0
4 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 14239 1
5 CPD-69 402 s*b 05 35 27.9799035534 -69 16 10.561668692   12.28 12.24 11.1   B3I 279 1
6 SN 1987A SN* 05 35 28.020 -69 16 11.07   4.75 4.81     SN.IIPec 4364 2
7 SN 1991G SN* 12 05 28.85 +50 32 11.7   15.7       SN.IIP 44 1
8 SN 2002hh SN* 20 34 44.29 +60 07 19.0     17.18     SN.IIP 128 1
9 NGC 6946 H2G 20 34 52.332 +60 09 13.24   10.5       ~ 2171 2

    Equat.    Gal    SGal    Ecl

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2019.09.17-13:21:25

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