In dense cores, much of the molecular material is frozen on the surface of dust grains. AKARI allows the simultaneous observation of multiple lines of site (los) through a core. We observed a 1’x1’ region towards 20 cores, between 2.5–5.0 μm. Data was reduced using our own pipeline (Noble et al. in prep.), producing spectra for 31 los
Context. Hot cores are signposts of the protostellar activity of dense cores in star-forming regions...
Paper presented at the American Astronomical Society Meeting #223 that took place in Washington, DC ...
Cryo-cell UV-LA-ICPMS is a new technique for direct chemical analysis of frozen ice cores at high s...
We present maps of the column densities of H2O, CO2 and CO ices towards the molecular cores B 35A, D...
Aims.Ices in dense star-forming cores contain the bulk of volatile molecules apart from H2 and thus ...
2.5-5 mu m spectra of four embedded protostars in the molecular core B35A were extracted using a nov...
The 11th Symposium on Polar Science/Ordinary sessions: [OM] Polar Meteorology and Glaciology, Poster...
Ice cores provide a robust reconstruction of past climate. However, development of timescales by an...
Five regions of massive-star formation have been observed in various molecular lines in the frequenc...
Polar ice cores play a central role in studies of the earth's climate system through natural archive...
Due to its micron-scale resolution and micro-destructiveness, laser ablation inductively coupled pla...
International audienceContext. A solar-type system starts from an initial molecular core that acquir...
2.5–5 μm spectra of four embedded protostars in the molecular core B35A were extracted using a novel...
Context. Hot cores are signposts of the protostellar activity of dense cores in star-forming regions...
Paper presented at the American Astronomical Society Meeting #223 that took place in Washington, DC ...
Cryo-cell UV-LA-ICPMS is a new technique for direct chemical analysis of frozen ice cores at high s...
We present maps of the column densities of H2O, CO2 and CO ices towards the molecular cores B 35A, D...
Aims.Ices in dense star-forming cores contain the bulk of volatile molecules apart from H2 and thus ...
2.5-5 mu m spectra of four embedded protostars in the molecular core B35A were extracted using a nov...
The 11th Symposium on Polar Science/Ordinary sessions: [OM] Polar Meteorology and Glaciology, Poster...
Ice cores provide a robust reconstruction of past climate. However, development of timescales by an...
Five regions of massive-star formation have been observed in various molecular lines in the frequenc...
Polar ice cores play a central role in studies of the earth's climate system through natural archive...
Due to its micron-scale resolution and micro-destructiveness, laser ablation inductively coupled pla...
International audienceContext. A solar-type system starts from an initial molecular core that acquir...
2.5–5 μm spectra of four embedded protostars in the molecular core B35A were extracted using a novel...
Context. Hot cores are signposts of the protostellar activity of dense cores in star-forming regions...
Paper presented at the American Astronomical Society Meeting #223 that took place in Washington, DC ...
Cryo-cell UV-LA-ICPMS is a new technique for direct chemical analysis of frozen ice cores at high s...