The Fermi LAT source 4FGL J1405.1-6119 is identified as a high-mass gamma-ray binary with a 13.7135-day period, confirmed by modulated gamma-ray, X-ray, and radio emission and an O6.5 III stellar counterpart.
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Discovery of the Galactic High-Mass Gamma-ray Binary 4FGL J1405.1-6119
The Fermi LAT source 4FGL J1405.1-6119 is identified as a high-mass gamma-ray binary with a 13.7135-day period, confirmed by modulated gamma-ray, X-ray, and radio emission and an O6.5 III stellar counterpart.