Eli Dwek

TL;DR: In this paper, the chemistry of silicate dust formation in AGN accretion disk winds is investigated. And the results indicate that these winds provide conditions conducive to the formation of significant amounts of dust, especially for objects accreting close to their Eddington limit, making AGNs a significant source of dust in the universe.

TL;DR: In this article, a simple expression for the rate at which the kinematically accessible paraboloid sweeps over the length of a thin uniform circular ring is derived, and a simple integral expression for a fluorescent line in terms of epsilon(t), the local line emissivity, is presented.

TL;DR: A quantitative analysis of the infrared emission of the supernova remnant Puppis A as seen by the Infrared Astronomical Satellite (IAS) is presented in this paper, where physical parameters of the remnant (and the surrounding interstellar medium) including density, mass, temperature, and age are estimated.

TL;DR: In this paper, a new radio image of the supernova remnant Puppis A and its surrounding medium was obtained with the IRAS and compared at radio, infrared, optical, and X-ray wavelengths.

TL;DR: In this article, the authors analyzed the far-ultraviolet (FUV) to near-infrared (near-IR) spectral energy distribution of seventeen 10 kpc diameter regions across the galaxy, and derived their star formation history, current star formation rate, and stellar population and mass.