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arXiv · 2208.08694

The integrated radio spectrum of G2.4$+$1.4

D. A. Green
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Abstract

The Galactic source G2.4$+$1.4 is an optical and radio nebula containing an extreme Wolf--Rayet star. At one time this source was regarded as a supernova remnant, because of its apparent non-thermal radio spectrum, although this was based on limited observations. Subsequent observations instead supported a flat, optically thin thermal radio spectrum for G2.4$+$1.4, and it was identified as a photoionized, mass-loss bubble, not a supernova remnant. Recently, however, it has been claimed that this source has a non-thermal integrated radio spectrum. I discuss the integrated radio flux densities available for G2.4$+$1.4 from a variety of surveys, and show that it has a flat spectrum at gigahertz frequencies (with a spectral index $\alpha$ of $0.02 \pm 0.08$, where flux density $S$ scales with frequency $\nu$ as $S \propto \nu^{-\alpha}$).

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D. A. Green. 2022-08-18. The integrated radio spectrum of G2.4$+$1.4. https://doi.org/10.1093/mnras%2Fstac2346

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