The discovery of WD 137 has sparked interest in further studies:
The PDF will begin with an abstract summarizing the discovery: "We present optical and ultraviolet spectroscopy of WD 137, a massive oxygen-neon white dwarf in a binary system..." You will learn the star’s mass (typically 0.8 to 1.2 solar masses), effective temperature, and any unusual composition. White Dwarf 137 Pdf
Issue 137 is highly regarded for its diverse range of articles covering both the fantasy and sci-fi universes: The discovery of WD 137 has sparked interest
Unlikely. Sirius B is usually designated by name, not a catalog number. "137" is almost certainly an entry number in a table. "137" is almost certainly an entry number in a table
The paper presents the discovery of a nearby white dwarf star, designated as WD 137, which has garnered significant attention in the astronomical community. Located approximately 27 parsecs (about 88 light-years) from Earth, WD 137 is one of the closest white dwarfs to the Sun. The authors of the paper, published in 2020, aim to characterize this star's properties, shedding light on its origin, evolution, and potential implications for our understanding of white dwarf formation and the local stellar population.
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A white dwarf no longer fuses elements. It shines from residual heat. The PDF will likely include a showing White Dwarf 137 on a cooling track. The age of the star (its cooling age) can be derived from its temperature and luminosity. This gives an independent age for the stellar population (e.g., the Galactic disk or halo).