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A Survey of Radio Recombination Line Emission From the Galactic Center Region
Symposium - International astronomical union
Preliminary results of a systematic survey of H78α, H91α and H98β emission from the inner 40′ of the Galactic center region are presented. This region consists of two prominent continuum features, the Sgr A complex and the radio continuum Arc. In spite of much nonthermal emission arising from these two features, we detected strong line emission with large line widths in more than half of the observed 130 positions. Many of the detections are new, in particular −50 km s−1 ionized gas linking thedoi:10.1017/s0074180900186474 fatcat:bx6jmsbvj5dwfighkoi2fjzdyq