The term "White Dwarf 137" is not a single, officially designated star (like Sirius B or Procyon B). Instead, it commonly refers to a catalog entry—often from survey data (such as the or a specific study code)—or a misdirected search for papers discussing hot white dwarfs with a temperature parameter of ~137,000 Kelvin. Alternatively, it may reference a numbered figure or table (Table 137) in a seminal PDF document, such as the Montreal White Dwarf Database or the Gaia DR3 white dwarf luminosity function .
in this context is an understatement. While our Sun’s surface is about 5,778 K, a young white dwarf can have surface temperatures exceeding 100,000 K to 200,000 K . These are the "hot" white dwarfs. They emit most of their radiation in the extreme ultraviolet (EUV) and soft X-ray bands. white dwarf 137 pdf hot
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"white dwarf" 137000 K PDF "white dwarf" "137" "hot" filetype:pdf "Teff = 137" white dwarf Filter by year (if you want recent models) or by author (e.g., Bergeron, Fontaine, Dufour). arXiv is the best source for free, complete PDFs. Search: The term "White Dwarf 137" is not a