Accurate Mass Determination of the Nearby Single White Dwarf L145 141 (LAWD 37) through Astrometric Microlensing

Kailash C Sahu,Jay Anderson,Andrea Bellini,Vasily Belokurov,Pierre Bergeron,Howard E Bond,Daniel Bramich,Thomas M Brown,Annalisa Calamida,Stefano Casertano,Martin Dominik, Wyn Evans,Noe Kains,Jonas Klueter,Peter McGill,Edmund Nelan,Martin Bo Nielsen,Richard Smart,Leigh Smith,Joachim Wambsganss

HST Proposal（2020）

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摘要

White dwarf (WD) is the final stage for a vast majority of stars, and WDs are important in a variety of astrophysical and galactic contexts. However, there are surprisingly few WDs with direct mass measurements, all of them in binaries.

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