J. A. CombiJ. F. Albacete-ColomboJ. López‐SantiagoGustavo E. RomeroE. Sánchez-AyasoJ. Martı́Pedro L. Luque‐EscamillaPablo G. Pérez‐GonzálezA. J. Muñoz‐ArjonillaJ. R. Sánchez-Sutil2026-03-222026-03-22201010.1051/0004-6361/200913735https://doi.org/10.1051/0004-6361/200913735https://andeanlibrary.org/handle/123456789/48516Citaciones: 15Aims. We report results of an X-ray study of the supernova remnant (SNR) G344.7-0.1 and the point-like X-ray source located at the geometrical center of the SNR radio structure. Methods. The morphology and spectral properties of the remnant and the central X-ray point-like source were studied using data from the XMM-Newton and Chandra satellites. Archival radio data and infrared Spitzer observations at 8 and 24 m were used to compare and study its multi-band properties at different wavelengths.enSupernova remnantX-rayPhysicsObject (grammar)Point (geometry)Point sourceCenter (category theory)AstrophysicsSupernovaAstronomyarticle