The observed orbit and elongation of the dusty source X7 are consistent with ejecta launched from the star S33/S0-30 in about 1950, favoring a grazing collision origin.
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Tidal phenomena in the Galactic Center: The curious case of X7
The observed orbit and elongation of the dusty source X7 are consistent with ejecta launched from the star S33/S0-30 in about 1950, favoring a grazing collision origin.