226 citations · 2.7k across the 57 of their papers we have counts for
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The LF of TP-AGB stars in the LMC and SMC
Gustavo Bruzual, Stephane Charlot, Rosa Gonzalez Lopezlira +3
We show that Montecarlo simulations of the TP-AGB stellar population in the LMC and SMC galaxies using the CB* models produce LF and color distributions that are in closer agreemen…
The Spatial Distribution of Dust and Stellar Emission of the Magellanic Clouds
Ramin A. Skibba, Charles W. Engelbracht, Gonzalo Aniano +24
We study the emission by dust and stars in the Large and Small Magellanic Clouds, a pair of low-metallicity nearby galaxies, as traced by their spatially resolved spectral energy d…
Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC). I. Overview
Karl D. Gordon, Margaret Meixner, Marilyn Meade +57
The Small Magellanic Cloud (SMC) provides a unique laboratory for the study of the lifecycle of dust given its low metallicity (~1/5 solar) and relative proximity (~60 kpc). This m…
On the origin of M81 group extended dust emission
J. I. Davies, C. D. Wilson, R. Auld +57
Galactic cirrus emission at far-infrared wavelengths affects many extragalactic observations. Separating this emission from that associated with extragalactic objects is both impor…
Radial distribution of gas and dust in the two spiral galaxies M99 and M100
M. Pohlen, L. Cortese, M. W. L. Smith +55
By combining Herschel-SPIRE data with archival Spitzer, HI, and CO maps, we investigate the spatial distribution of gas and dust in the two famous grand-design spirals M99 and M100…
Probing the molecular interstellar medium of M82 with Herschel-SPIRE spectroscopy
P. Panuzzo, N. Rangwala, A. Rykala +60
We present the observations of the starburst galaxy M82 taken with the Herschel SPIRE Fourier Transform Spectrometer. The spectrum (194-671 μm) shows a prominent CO rotational ladd…