Robert E. Stencel

TL;DR: In this article, the authors reported interferometric images that show the eclipsing body moving in front of the B5V-type star, and they derived a mass of approximately (3.6 +/- 0.7)M for the F star.

TL;DR: In this article, a simple model of the expected Kuiper Belt (KB) small grain population and the thermal emission that would arise from such grains was proposed and the model assumed equilibrium between grain creation by collisional fragmentation of comets and removal by Poynting-Robertson radiation drag, radiation pressure-driven ejection, mutual collisions, and sublimation.

TL;DR: In this article, the first results of the MIRIAD (MIPS InfraRed Imaging of AGB Dust shells) project using the Spitzer Space Telescope were presented.

TL;DR: In this paper, the spectral energy distribution (SED) of the Aurigae binary star was modeled using a three-component model consisting of a 2.2^(+0.9)_(−0.8) M_☉ F-type post-asymptotic giant branch star, and a 5.9 ± 0.8 M_ℓ B5±1 type main-sequence star.

TL;DR: In this article, an extension of the previous analysis of infrared excesses among a volume-limited sample of 134 nearby A-K main-sequence stars to a magnitude limited sample of stars, culled from the SAO catalog, with excesses determined from the IRAS Point Source Catalog flux density ratios.