226 citations · 2.7k across the 51 of their papers we have counts for
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Ice chemistry in massive Young Stellar Objects: the role of metallicity
J. M. Oliveira, J. Th. van Loon, G. C. Sloan +6
We present the comparison of the three most important ice constituents (water, CO and CO2) in the envelopes of massive Young Stellar Objects (YSOs), in environments of different me…
Infrared properties of Active OB stars in the Magellanic Clouds from the Spitzer SAGE Survey
A. Z. Bonanos, D. J. Lennon, D. L. Massa +9
We present a study of the infrared properties of 4922 spectroscopically confirmed massive stars in the Large and Small Magellanic Clouds, focusing on the active OB star population.…
The mass-loss return from evolved stars to the Large Magellanic Cloud III. Dust properties for carbon-rich asymptotic giant branch stars
Sundar Srinivasan, B. A. Sargent, M. Matsuura +9
We present a 2Dust model for the dust shell around a LMC long-period variable (LPV) previously studied as part of the OGLE survey. OGLE LMC LPV 28579 (SAGE J051306.40-690946.3) is…
Herschel Observations of a Newly Discovered UX Ori Star in the Large Magellanic Cloud
Geoffrey C. Clayton, B. Sargent, M. L. Boyer +15
The LMC star, SSTISAGE1C J050756.44-703453.9, was first noticed during a survey of EROS-2 lightcurves for stars with large irregular brightness variations typical of the R Coronae…
Cold dust clumps in dynamically hot gas
S. Kim, E. Kwon, S. C. Madden +27
We present clumps of dust emission from Herschel observations of the Large Magellanic Cloud (LMC) and their physical and statistical properties. We catalog cloud features seen in t…
Dust in the bright supernova remnant N49 in the LMC
M. Otsuka, J. Th. van Loon, K. S. Long +14
We investigate the dust associated with the supernova remnant (SNR) N49 in the Large Magellanic Cloud (LMC) as observed with the Herschel Space Observatory. N49 is unusually bright…