SIMBAD references

2011ApJ...743....4Z - Astrophys. J., 743, 4 (2011/December-2)

Molecular environment and an X-ray spectroscopy of supernova remnant Kesteven 78.

ZHOU P. and CHEN Y.

Abstract (from CDS):

We investigate the molecular environment of the Galactic supernova remnant (SNR) Kesteven 78 and perform an XMM-Newton X-ray spectroscopic study for the northeastern edge of the remnant. SNR Kes 78 is found to interact with the molecular clouds (MCs) at a systemic local standard of rest velocity of 81 km/s. At around this velocity, the SNR appears to contact a long molecular strip in the northeast and a large cloud in the east as revealed in the 13CO line, which may be responsible for the radio brightness peak and the OH maser, respectively. The 12CO-line bright region morphologically matches the eastern bright radio shell in general, and the SNR is consistent in extent with a CO cavity. Broadened 12CO-line profiles discerned in the eastern maser region and the western clumpy molecular arc and the elevated 12CO (J = 2-1)/(J = 1-0) ratios along the SNR boundary may be signatures of shock perturbation in the molecular gas. The SNR-MC association places the SNR at a kinematic distance of 4.8 kpc. The X-rays arising from the northeastern radio shell are emitted by underionized hot (∼1.5 keV), low-density (∼0.1/cm3) plasma with solar abundance, and the plasma may be of intercloud origin. The age of the remnant is inferred to be about 6 kyr. The size of the molecular cavity in Kes 78 implies an initial mass around 22 M for the progenitor.

Abstract Copyright:

Journal keyword(s): ISM: individual: G32.8-0.1 = Kes 78 - ISM: molecules - ISM: supernova remnants

Simbad objects: 10

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2011ApJ...743....4Z and select 'bookmark this link' or equivalent in the popup menu


2021.03.06-06:13:11

© Université de Strasbourg/CNRS

    • Contact