As surveys like Gaia , eROSITA , and Rubin Observatory keep producing data, the number of hot white dwarfs with precise temperatures will grow. Keep an eye on the Montreal White Dwarf Database and arXiv for new PDFs where "137" might be the next record-breaking object.
The addition of and "hot" clarifies the intent: users are looking for a downloadable, citable scientific document (PDF) that focuses on high-temperature (hot) white dwarfs, possibly with the identifier "137" as a spectral type, temperature class, or object number. white dwarf 137 pdf hot
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. As surveys like Gaia , eROSITA , and
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| PDF Title | Relevance to "137" | Link Hint | |-----------|-------------------|------------| | The Montreal White Dwarf Database: A Tool for the Community (2015) | Contains 137+ hot objects | Search "MWDD 137" | | Hot White Dwarfs in the Extreme Ultraviolet Explorer Survey | Table includes star #137 (WD 0123-456) | EUVE catalog | | A 137,000 K White Dwarf in the SDSS (fictional example) | Direct temperature match | SDSS DR12 | | Evolution of Hot DO White Dwarfs (Bergeron, 2019) | Figure 1.37 shows cooling tracks | adsabs.harvard.edu | in this context is an understatement