Rd. Oudmaijer et al., DISCOVERY OF NEAR-INFRARED HYDROGEN LINE EMISSION IN THE PECULIAR F8 HYPERGIANT IRC+10420, Astronomy and astrophysics, 281(1), 1994, pp. 33-36
High resolution infrared spectroscopy of IRC +10420 has revealed remar
kable profiles of several hydrogen recombination lines, with emission
detected for the first time in these lines. Brgamma, Pfgamma and Bralp
ha have emission peaks blue-shifted with respect to the photosphere, B
r12 shows an emission core in the photospheric absorption line. In con
trast, the Halpha line profile is double peaked. The line emission is
interpreted as originating from a bipolar outflow that probably starte
d as recent as ten years ago.