White Dwarf 137 Pdf Hot -

Retro Review: Why White Dwarf 137 (May 1991) Still Matters If you're scouring the web for a "White Dwarf 137 PDF," you’re likely chasing a specific kind of tabletop nostalgia. Released in , Issue 137 is a quintessential piece of Games Workshop history

2. Physical Parameters of WD 137 (SDSS J1240+6715)

According to data compiled from peer-reviewed PDF documents and the Gaia Early Data Release 3 (EDR3), the key parameters of this object are: white dwarf 137 pdf hot

3.3 Pulsations and Asteroseismology

The hottest white dwarfs (known as GW Vir stars, after the variable star GW Virginis) pulsate. These are stars in the PG 1159 spectral class. A "137" reference might appear in: Retro Review: Why White Dwarf 137 (May 1991)

Possibility 4: Spectral Type "Hot DQ" or "Hot DZ" – with subclass 137

Some non-DA white dwarfs have carbon (DQ) or metal (DZ) lines. A hot DQ white dwarf with a temperature of ~137,000 K would be a unique object. The number 137 might appear in the Montreal white dwarf cooling models as a specific grid point. Many astrophysics PDFs use numbers like “137” as

• Many astrophysics PDFs use numbers like “137” as volume, page, or article identifiers. Example: recent papers on hot or unusually hot white dwarfs appear in journals (e.g., PASP, ApJ) and as arXiv preprints; their PDF filenames or article codes sometimes include numbers (e.g., “PASP 137 …pdf”).
• If you meant a specific paper titled or numbered with “137”, give the full bibliographic detail; otherwise search results that include “137” often point to journal volumes or article numbers rather than a canonical “White Dwarf 137” object.

If you want, I can:

Look for paper IDs like arXiv:1506.08237 (note "137" at the end). For example:

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