Article citationsMore>>

Koralesky, B., Frail, D.A., Goss, W.M., Claussen, M.J. and Green, A.J. (1998) Shock- Excited Maser Emission from Supernova Remnants: G32.8-0.1, G337.8-0.1, G346.6- 0.2, and the HB 3/W3 Complex. The Astronomical Journal, 116, 1323-1331.
https://doi.org/10.1086/300508

has been cited by the following article:

• TITLE: Multipole Analysis of Radio Continuum Images of Supernova Remnants: Comparison of Type Ia and Core Collapse

  AUTHORS: Sujith Ranasinghe, Denis Leahy

  KEYWORDS: Supernova Remnants, Radio Continuum, Radio Lines

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.5 No.3, July 16, 2019

  ABSTRACT: A multipole expansion analysis is applied to 1420 MHz radio continuum images of supernova remnants (SNRs) in order to compare Type Ia and core collapse (CC) SNRs. Because the radio synchrotron emission is produced at the outer shock between the SNR and the ISM, we are investigating whether the ISM interaction of SNRs is different between Type Ia and CC SNRs. This is in contrast to previous investigations, which have shown that Type Ia and CC SNRs have different asymmetries in the X-ray emission from their ejecta. The sample consists of 19 SNRs which have been classified as either Type Ia or CC. The quadrupole and octupole moments normalized to their monopole moments (total emission) are used as a measure of asymmetry of the emission. A broad range (by a factor of ~1000) is found for both quadrupole and octupole normalized moments. The strongest correlation we find is that large quadrupole moments are associated with large octupole moments, indicating that both serve as similar indicators of asymmetry. The other correlation we find is that both moments increase with SNR age or radius. This indicates that interstellar medium structure is a strong contributor to asymmetries in the radio emission from SNRs. This does not seem to apply to molecular clouds, because we find that association of a SNR with a molecular cloud is not correlated with larger quadrupole or octupole moments.