The supernova remnant in 30 DOR B

Details The supernova remnant in 30 DOR B The supernova remnant in 30 DOR B

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.195p..33d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 195, May 1981, p. 33P-37P.

Astronomy and Astrophysics

Astronomy

26

Astronomical Photography, Astronomical Spectroscopy, Radio Sources (Astronomy), Radio Spectra, Supernova Remnants, X Ray Sources, X Ray Spectra, Bandpass Filters, Crab Nebula, Emission Spectra, H Alpha Line, Iron, Line Spectra, Magellanic Clouds, Spectrum Analysis

Scientific paper

An optical counterpart of the radio/X-ray supernova remnant in 30 Dor B
in the LMC has been detected by direct imaging and spectroscopic
techniques. Interesting properties at X-ray, optical and radio
wavelengths are considered. Because it has a non-thermal X-ray spectrum
and a flat radio spectrum, it may be a Crab-like SNR, but more evolved.

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