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In astronomy, stars are often cataloged by number. white dwarf 137 pdf hot
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Finding a high-quality scan of White Dwarf 137 is a bit like finding an artifact in a tomb. Physical copies are brittle and expensive, making the digital version the best way to experience this slice of history. The blackbody peak for a 90,000 K object
The blackbody peak for a 90,000 K object lies in the extreme ultraviolet (around 30 nm). This EUV radiation can photoevaporate any circumstellar material, such as a debris disk.
A white dwarf with Teff = 137,000 K . A search for "white dwarf 137000 K" yields numerous PDFs. For example, the famous hot white dwarf PG 1159-035 (the prototype of the PG 1159 spectral class) has Teff ~140,000 K, close to 137 kK. Similarly, RX J0439.8-6809 – one of the hottest known (up to 250,000 K) – is often cited in tables that include row #137.
LP 137-14 is a known high-mass white dwarf (0.85 solar masses) located in the Galactic halo. While its number is "137," it is a high-proper-motion star. Recent Gaia PDFs show it has a temperature of 98,000 K and a peculiar atmosphere polluted by heavy elements.