Discovery of a new supergiant fast X-ray transient MAXI J0709-159 associated with the Be star LY Canis Majoris

We report on the discovery of a new supergiant fast X-ray transient (SFXT), MAXI J0709-159, and its identification with LY CMa (also known as HD 54786). On 2022 January 25, a new flaring X-ray object, named MAXI J0709-159, was detected by the Monitor of All-sky X-ray Image (MAXI). Two flaring activities were observed in two scans similar to 3 hr apart, where the 2-10 keV flux reached 5 x 10(-9) erg cm(-2) s(-1). During the period, the source exhibited a large spectral change, suggesting that the absorption column density N-H increased from 10(22) to 10(23) cm(-2). A NuSTAR follow-up observation on January 29 identified a new X-ray source with a flux of 6 x 10(-13) erg cm(-2) s(-1) at a position consistent with LY CMa, which has been identified as a B supergiant as well as a Be star, located at a 3 kpc distance. The observed X-ray activity, characterized by short (less than or similar to several hours) duration, rapid (less than or similar to a few seconds) variabilities accompanied by spectral changes, and a large luminosity swing (10(32)-10(37) erg s(-1)), agree with those of SFXTs. On the other hand, optical spectroscopic observations of LY CMa reveal a broad H alpha emission line, which may indicate the existence of a Be circumstellar disk. These results suggest that the optical companion, LY CMa, certainly has a complex circumstellar medium including dense clumps.