Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer
Ellyn K. Baines, J. Thomas Armstrong, Henrique R. Schmitt, R. T., Zavala, James A. Benson, Donald J. Hutter, Christopher Tycner, and Gerard T., van Belle

TL;DR
This paper reports precise fundamental stellar parameters for 87 stars, including 36 newly measured via optical interferometry, covering a wide spectral range and providing key data for stellar characterization.
Contribution
It provides new interferometric angular diameter measurements for 36 stars and derives comprehensive physical properties, enhancing stellar parameter databases.
Findings
36 stars measured for the first time using interferometry.
Derived stellar radii, temperatures, and luminosities for all 87 stars.
Sample includes a diverse range of spectral types from B to M.
Abstract
We present the fundamental properties of 87 stars based on angular diameter measurements from the Navy Precision Optical Interferometer, 36 of which have not been measured previously using interferometry. Our sample consists of 5 dwarfs, 3 subgiants, 69 giants, 3 bright giants, and 7 supergiants, and span a wide range of spectral classes from B to M. We combined our angular diameters with photometric and distance information from the literature to determine each star's physical radius, effective temperature, bolometric flux, luminosity, mass, and age.
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