2011A&A...527A..55P


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.04CEST01:51:58

2011A&A...527A..55P - Astronomy and Astrophysics, volume 527A, 55-55 (2011/3-1)

The Cygnus Loop: a weak core-collapse SN in our galaxy.

PREITE MARTINEZ A.

Abstract (from CDS):

The Cygnus Loop is thought to be the result of a core-collapse supernova (SN) explosion in the cavity formed by the wind of the progenitor star. Since then the shock has run through the low-density cavity, hit the cavity wall, and it is now running into a denser environment. We test the consistency of the global parameters of the remnant (as derived at the cavity-cloud interface) with the observational scenario in the north-east (NE) sector of the remnant. The test is performed with the help of a time-dependent spherically-symmetric hydrodynamical (HD) code using a smooth density distribution at the cavity-cloud interface. When the shock hits the wall of the cavity, the reflected perturbation is found not to be a shock wave but a strong compression wave. The reflected wave heats up the cavity at temperatures higher than those observed in the X-rays. We also find an outwardly decreasing temperature as observed in X-rays, but over a narrower radial interval. After crossing the wall of the cavity, the shock velocity in the cloud is not steady. Nonetheless, we find that the steady-state assumption usually made to fit the line emission of Balmer-dominated non-radiative filaments (NRFs) can be rather accurate (shock velocity variations <3%) if the integration time of the post-shock structure is shorter than ∼200y, the shock is not too close to the wall and the cloud was not shocked more than ∼1100yr ago. We propose a revision of the parameters of the cavity-wall scenario, assuming as a constraint the approximate steadiness of the shock velocity in the cloud. With the revised set of parameters, the values of the temperature in the hot cavity are in closer agreement with observations. At the adopted distance of 540 pc, we find an explosion energy E0≃6-8x1049erg, consistent with previous determinations of E0 once scaled to the adopted distance. We also determine lower and upper limits of 0.1 and 2.6x1050erg. This very low value of E0 suggests an electron-capture explosion of an ∼8-10M progenitor, and makes the SN of the Cygnus Loop the weakest known core-collapse SN in the Galaxy.

Abstract Copyright:

Journal keyword(s): ISM: supernova remnants - ISM: individual objects: Cygnus Loop - supernovae: general - hydrodynamics - shock waves

Simbad objects: 5

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Number of rows : 5

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 SN 2005E SN* 02 39 14.34 +01 05 55.0     16.8     SNIb/c 104 1
2 V* CM Tau Psr 05 34 31.93830 +22 00 52.1758           ~ 4803 1
3 M 51 GiP 13 29 52.698 +47 11 42.93   9.26 8.36 8.40   ~ 3781 4
4 SN 2005cs SN* 13 29 53.37 +47 10 28.2   14.5       SNIIP 329 1
5 NAME Cyg Loop SNR 20 51.0 +30 40           ~ 822 0

    Equat.    Gal    SGal    Ecl

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2020.07.04-01:51:58

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