activity
19942025
most citedSpitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results

718 citations · 6.5k across the 104 of their papers we have counts for

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Showing 2008Show all

7 papers · 1 filter

astro-ph2008★ 52 cited

A spatially resolved study of photoelectric heating and [CII] cooling in the LMC

D. Rubin, S. Hony, S. C. Madden +20

(abridged) We study photoelectric heating throughout the Large Magellanic Cloud. We quantify the importance of the [CII] cooling line and the photoelectric heating process of vario…

astro-ph2008★ 58 cited

Variable Evolved Stars and YSOs Discovered in the Large Magellanic Cloud using the SAGE Survey

Uma P. Vijh, M. Meixner, B. Babler +13

We present initial results and source lists of variable sources in the Large Magellanic Cloud (LMC) for which we detect thermal infrared variability from the SAGE (Surveying the Ag…

astro-ph2008★ 61 cited

Photometry using the Infrared Array Camera on the Spitzer Space Telescope

Joseph L. Hora, Sean Carey, Jason Surace +13

We present several corrections for point source photometry to be applied to data from the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. These corrections are necessa…

astro-ph2008★ 155 cited

Clustered and Triggered Star Formation in W5: Observations with Spitzer

Xavier P. Koenig, Lori E. Allen, Robert A. Gutermuth +3

We present images and initial results from our extensive Spitzer Space Telescope imaging survey of the W5 H II region with the Infrared Array Camera (IRAC) and Multiband Imaging Ph…

astro-ph2008★ 19 cited

Radio continuum properties of young planetary nebulae

L. Cerrigone, G. Umana, C. Trigilio +3

We have selected a small sample of post-AGB stars in transition towards the planetary nebula and present new Very Large Array multi-frequency high-angular resolution radio observat…

astro-ph2008★ 3 cited

Planetary Nebulae: Exposing the Top Polluters of the ISM

Joseph L. Hora, Massimo Marengo, Howard A. Smith +2

The high mass loss rates of stars in their asymptotic giant branch (AGB) stage of evolution is one of the most important pathways for mass return from stars to the ISM. In the plan…