Great surplus firearm! In used but really good condition. SHIPPING CHARGES WILL BE APPLIED UPON SHIPPING. PLEASE NOTE: FREE SHIPPING PROMOTIONS DO NOT APPLY TO FIREARMS ORDERS. NO EXCEPTIONS.ĪLL PISTOLS NOT FOR SALE IN MASSACHUSETTS OR MARYLAND (PLEASE CHECK LOCAL LAWS) This is a stock photo, actual firearm may vary.īEFORE PLACING AN ORDER FOR A FIREARM, PLEASE CLICK HERE TO READ OUR FIREARMS ORDERING INFORMATION TO AVOID HAVING YOUR ORDER CANCELEDįFL REQUIRED AT TIME OF PURCHASE. Buy with a gun purchase per 100rds! (9x23mm or what is called 9mm Largo ) Use Part#AM195.ĭUE TO LOW STOCK NO PURCHASES OVER 500 ROUNDSĪMMUNITION MUST BE PURCHASED SEPARATELY FROM THE PISTOL This is the 'A' model with the 5 inch barrel and in Fair - Good condition. 38 Super auto! We bought 6,000 of these from Interarms 20 years ago and this cache was forgotten about in our vast inventory tucked away in the recesses of the Firearms bunker. Our K-band speckle-imaging data reveal the star to be single down to a projected separation of 110 AU.A Lost Piece of History Revealed Deep in the Bunker! We interpret the star and its surrounding nebula as an LBV that has recently ejected large amounts of material. This is consistent with our evolutionary models, which predict that the star is in an unstable evolutionary stage. The inferred luminosity and temperature place the star in a sparsely populated zone in the H-R diagram where luminous blue variables (LBVs) are often found. As previously existing stellar evolution models do not extend to such high luminosities, we employ new evolutionary tracks for very massive stars to determine the initial mass and age of the Pistol Star, and estimate M initial = 200-250 M ⊙ and an age of 1.7-2.1 Myr. The models also reveal a helium enriched surface. The lower luminosity models give L = 10 6.6+/-0.2 L ⊙ and T eff = 10 4.15+/-0.01 K, while the higher luminosity models give L = 10 7.2+/-0.2 L ⊙ and T eff = 10 4.33+/-0.01 K the error in luminosity assumes an uncertainty of +/-0.5 in A K, while the error in T eff is constrained by detailed line modeling. Using our wind/atmosphere code, we find two families of models that fit the spectral energy distribution and detailed line profiles. We estimate an extinction of A K = 3.2 +/- 0.5 using the near-infrared colors of the star and of surrounding stars in the young Quintuplet cluster. We present new near-infrared data and analysis, which indicate that the Pistol Star is one of the most luminous stars known, adding another test point for massive star formation and stellar evolution theories.
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