A new class of radio star

Details A new class of radio star A new class of radio star

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978natur.276..571r&link_type=abstract

Nature, vol. 276, Dec. 7, 1978, p. 571-573.

Astronomy and Astrophysics

Astronomy

70

Radiant Flux Density, Radio Stars, Stellar Evolution, Supernova Remnants, Extragalactic Radio Sources, Light Emission, Point Sources, Radio Astronomy, X Ray Sources

Scientific paper

Radio observations of the point radio source 1909+048 indicate that this entity, which is in W50, is a distinct new type of radio source. It is suggested that the source is the stellar remains of a supernova. Characteristics of possibly similar sources are reported, and flux density patterns over time are presented for some of the sources. It is noted that the radio properties of the new class are superficially similar to the properties of some extragalactic sources, the BL Lac objects, and the possibility is considered that some of the proposed sources are incorrectly associated with stellar remnants of supernovas.

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