Page 3: Research news on X-ray astronomy

X-ray astronomy is the research area focused on detecting, imaging, and spectroscopically analyzing cosmic sources of X-ray photons, typically in the energy range of ~0.1–100 keV. Because Earth’s atmosphere is opaque to X-rays, this field relies on space-based observatories employing grazing-incidence optics, focusing telescopes, and high-resolution detectors such as CCDs, microcalorimeters, and proportional counters. X-ray astronomy probes high-energy astrophysical processes, including accretion onto compact objects, hot intracluster gas, supernova remnants, stellar coronae, and relativistic jets, enabling quantitative studies of extreme environments, plasma conditions, strong gravity, and energetic feedback in galaxies and large-scale structure.

Einstein Probe detects an X-ray flare from nearby star

Using the Einstein Probe (EP), astronomers have detected a new X-ray transient event, which turned out to be an X-ray flare from the star PM J23221-0301 located about 150 light years away. The finding was reported in a research ...

Image: JWST captures colliding spiral galaxies

Mid-infrared observations from NASA's James Webb Space Telescope, shown in white, gray, and red, are combined here with X-ray data from NASA's Chandra X-ray Observatory, highlighted in blue. Together, these different wavelengths ...

XMM-Newton sees comet 3I/ATLAS in X-ray light

The European Space Agency's X-ray space observatory XMM-Newton observed interstellar comet 3I/ATLAS on 3 December for around 20 hours. During that time, the comet was about 282–285 million km from the spacecraft.

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