Some PDFs report null detections of magnetic fields (less than 100 kG) for EG 267, which helps set limits on fossil magnetic field origins in single white dwarfs.
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White Dwarf 267 PDF is a highly sought-after document related to astronomy, specifically focusing on white dwarf stars. White dwarfs are remnants of low-mass stars that have exhausted their fuel and shed their outer layers. This guide aims to provide an overview of the content typically found in White Dwarf 267 PDF, along with an understanding of white dwarfs and their significance in astrophysics.
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