New Optical and X-Ray Observations Yield Progress in Understanding of an Old Nova / Nova Aquilae 1918

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Nova Aquilae 1918 was the brightest new star that was discovered since Tycho's and Kepler's supernovae in 1572 and 1604, which reached a peak brightness of -4^m and -3^m,respectively. On June 10, 1918, Nova V603 Aquilae went through a sharp maximum of visual brightness -1 ^m.1, followed by a subsequent steep decrease, making it an outstanding example of a classical fast nova. Consequently, it has been the sUbject of many investigations.

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