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Constraints on the Properties of Warm Ionized Gas from Low-frequency Hydrogen Radio Recombination Lines

  • Authors: Pedro Salas, Kimberly L. Emig, Matteo Luisi, D. Anish Roshi, Loren D. Anderson

Pedro Salas et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 3.

GDIGS RRL spectra toward G15.85+0.10 (left), G24.07−0.59 (center), and G31.00−0.91 (right) using three different beam sizes, ﹩36^{\prime} ﹩, ﹩16^{\prime} ﹩, and ﹩2\mathop{.}\limits{^{\prime} }65﹩. From top to bottom each row shows the GDIGS spectra at ﹩36^{\prime} ﹩ resolution, the GDIGS spectra at ﹩16^{\prime} ﹩ resolution, the difference between the GDIGS spectra at ﹩36^{\prime} ﹩ and ﹩16^{\prime} ﹩ resolutions, the GDIGS spectra at ﹩2\mathop{.}\limits{^{\prime} }65﹩ resolution, and the difference between the GDIGS spectra at ﹩16^{\prime} ﹩ and ﹩2\mathop{.}\limits{^{\prime} }65﹩ resolutions. The dotted lines show the 3σ rms of the differences. No scaling has been applied to compute the differences.

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