We present very early photometric and spectroscopic observations of the Type Ia supernova (SN Ia) 2023bee. starting about 8 hr after the explosion. which reveal a strong excess in the optical and nearest UV ( U and UVW1 ) bands during the first several days of explosion. This data set allows us to probe the nature of the binary companion of the exploding white dwarf and the conditions... https://www.bekindtopets.com/limited-offer-Sac-Mira-Grand-Cru-on-sale/