activity
19952023
most citedSpitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results

718 citations · 7.3k across the 122 of their papers we have counts for

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29 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★ 76 cited

HST Snapshot Survey of Post-AGB Objects

N. Siodmiak, M. Meixner, T. Ueta +3

The results from a Hubble Space Telescope (HST) snapshot survey of post-AGB objects are shown. The aim of the survey is to complement existing HST images of PPN and to connect vari…

astro-ph2007★ 46 cited

SPITZER SAGE Observations of Large Magellanic Cloud Planetary Nebulae

J. L. Hora, M. Cohen, R. G. Ellis +14

We present IRAC and MIPS images and photometry of a sample of previously known planetary nebulae (PNe) from the SAGE survey of the Large Magellanic Cloud (LMC) performed with the S…

astro-ph2007★ 77 cited

The Stellar Mass Distribution in the Giant Star Forming Region NGC 346

E. Sabbi, M. Sirianni, A. Nota +8

Deep F555W and F814W Hubble Space Telescope ACS images are the basis for a study of the present day mass function (PDMF) of NGC346, the largest active star forming region in the Sm…

astro-ph2007★ 38 cited

HST/NICMOS Imaging Polarimetry of Proto-Planetary Nebulae II: Macro-morphology of the Dust Shell Structure via Polarized Light

Toshiya Ueta, Koji Murakawa, Margaret Meixner

The structure of the dusty circumstellar envelopes (CSEs) of proto-planetary nebulae (PPNs) reveals the mass-loss history of these sources and how such histories may differ for ell…