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5 papers · 2 filters
Dense Clumps in Giant Molecular Clouds in the Large Magellanic Cloud: Density and Temperature Derived from CO() Observations
Tetsuhiro Minamidani, Takanori Tanaka, Yoji Mizuno +17
In order to precisely determine temperature and density of molecular gas in the Large Magellanic Cloud, we made observations of optically thin CO() transition by usin…
Herschel Inventory of The Agents of Galaxy Evolution (HERITAGE): the Large Magellanic Cloud dust
M. Meixner, F. Galliano, S. Hony +52
The HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE) of the Magellanic Clouds will use dust emission to investigate the life cycle of matter in both the Large and Sm…
Dust/gas correlations from Herschel Observations
Julia Roman-Duval, Frank P. Israel, Alberto Bolatto +21
Spitzer and IRAS observations of the LMC suggest an excess of FIR emission with respect to the gas surface density traced by 12CO and HI 21 cm emission lines. This "FIR excess" is…
Variations in the Na-O anticorrelation in globular clusters: Evidence for a deep mixing episode in red giant branch stars
Jae-Woo Lee
The Na-O anticorrelation seen in almost all globular clusters ever studied using high-resolution spectroscopy is now generally explained by the primordial pollution from the first…
The Solar Nebula on Fire: A Solution to the Carbon Deficit in the Inner Solar System
Jeong-Eun Lee, Edwin A. Bergin, Hideko Nomura
Despite a surface dominated by carbon-based life, the bulk composition of the Earth is dramatically carbon poor when compared to the material available at formation. Bulk carbon de…