High-resolution spectroscopy of standard stars and the FU Orionis-type object V960 Mon
Sunkyung Park
Konkoly Observatory
Hungary


Since most of the objects that make up the Galaxy are low-mass stars, investigation of low-mass stars is required to understand the Universe. To investigate the low-mass stars, we conducted a high-resolution near-infrared spectral library of various types of standard stars and provided template spectra. These stellar spectra are applied for the analysis of low-mass young stellar objects. In this talk, I will present the results of the IGRINS spectral library and its application to the FU Orionis-type object, V960 Mon.

Here you can play back the recording of the presentation