Abstract:We performed spectroscopic and photometric analyses on the early B‐type LP Ori young stellar object located in the Orion Nebula. The high‐resolution spectra of LP Ori was obtained at the Ankara University Kreiken Observatory in 2023, while all spectra recorded over the past 19 years were extracted from the ESO and ESPaDOnS archives. In these spectra of LP Ori, there is typically an emission observed in the core of the Balmer profile. This structure is accompanied by a 14‐year interval inverse P‐Cygni repetitio… Show more
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