Joseph L. Hora

TL;DR: In this article, the spectral energy distribution of stars with the strongest IR excess was modeled and a total cluster dust mass-loss rate of 3.0{sup +2.0}{sub -1.2} x 10{sup -9} M{sub sun} yr{sup −1, corresponding to a gas mass loss rate of 8.6

TL;DR: In this paper, the authors observed the nearby starburst galaxy NGC 253 in the mid-infrared to obtain a three-dimensional data set with arcsecond angular resolution and 0.2 km spectral resolution.

TL;DR: In this article, the authors report sub-arcsecond imaging of extended mid-infrared emission from a proto-planetary nebula (PPN), which is performed at the MMT observatory with its newly upgraded 6.5 m aperture telescope and at the Keck observatory.

TL;DR: In this article, an upper-limit flux density determination from the Spitzer Space Telescope Infrared Array Camera observations of near-Earth object 2009 BD was performed in support of the NASA Asteroid Robotic Retrieval Mission concept.

TL;DR: In this paper, the location of an individual PN in the color-color diagrams is seen to depend on the relative contributions of the spectral components which include molecular hydrogen, polycyclic aromatic hydrocarbons (PAHs), infrared forbidden line emission from the ionized gas, warm dust continuum, and emission directly from the central star.