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Multi-frequency Study of the LMC Supernova Remnant (SNR) B0513-692 and New SNR Candidate J051327-6911
I. S. Bojicic, M. D. Filipovic, Q. A. Parker +5
We present a new multi-wavelength study of supernova remnant (SNR) B0513-692 in the Large Magellanic Cloud (LMC). The remnant also has a strong, superposed, essentially unresolved,…
Multiwavelength appearance of Vela Jr.: Is it up to expectations?
A. F. Iyudin, B. Aschenbach, V. Burwitz +4
Vela Jr. is one of the youngest and likely nearest among the known galactic supernova remnants (SNRs). Discovered in 1997 it has been studied since then at quite a few wavelengths,…
A Statistical Study of Galactic SNRs using the PMN Survey
M. Stupar, M. D. Filipovic, Q. A. Parker +3
The Parkes-MIT-NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic Supernova Remnants (SNRs) at a common frequency of 4.85 GHz. We present flux dens…
G315.1+2.7: a new Galactic SNR from the AAO/UKST HAlpha survey
M. Stupar, Q. A. Parker, M. D. Filipovic
New narrow-band HAlpha imaging and subsequent optical spectra confirm G315.1+2.7, a previously identified candidate supernova remnant (SNR), as a bona-fide Galactic SNR. Present ob…
A multi-resolution analysis of the radio-FIR correlation in the Large Magellanic Cloud
A. Hughes, T. Wong, R. Ekers +5
We investigate the local correlation betwen the 1.4 GHz radio continuum and 60 micron far-infrared (FIR) emission within the Large Magellanic Cloud (LMC) on spatial scales between…
AGN in the XMM-Newton first-light image as probes for the interstellar medium in the LMC
F. Haberl, K. Dennerl, M. D. Filipovic +3
The XMM-Newton first-light image revealed X-ray point sources which show heavily absorbed power-law spectra. The spectral indices and the probable identification of a radio counter…