Add to ORKG2.5-5 mu m spectra of four embedded protostars in the molecular core B35A were extracted using a novel data reduction pipeline developed for AKARI near infrared (NIR) grism spectroscopy. Column densities of the solid phase species present in the four lines of sight were calculated, illustrating the sensitivity of AKARI. The importance of ice spectra of low luminosity protostars to the development of star formation theories is discussed
In dense cores, much of the molecular material is frozen on the surface of dust grains. AKARI allows...
Context. Starless cores represent a very early stage of the star formation process, before collapse...
International audienceContext. A solar-type system starts from an initial molecular core that acquir...
2.5-5 mu m spectra of four embedded protostars in the molecular core B35A were extracted using a nov...
2.5–5 μm spectra of four embedded protostars in the molecular core B35A were extracted using a novel...
We present near-infrared spectroscopic observations of 19 molecular clouds made using the AKARI sate...
34 pages, 9 figuresInternational audienceAbstract We present near-infrared spectra of three low-lumi...
To investigate the composition and evolution of circumstellar ice around low-mass young stellar obje...
Context. Circumstellar disks and envelopes of low-mass young stellar objects (YSOs) contain signific...
Circumstellar disks and envelopes of low-mass YSOs contain significant amounts of ice. Such icy mate...
Oral presentation given at the Terzo Workshop sull'Astronomia millimetrica e submillimetrica in Ital...
We present observations of L1155 and L1148 in the Cepheus molecular cloud, taken using the Far Infra...
Class 0 objects, which are thought to be the youngest protostars, are identified in terms of NIR or ...
The early stages of the formation of a planetary system are represented by Solar-type protostars. Re...
In dense cores, much of the molecular material is frozen on the surface of dust grains. AKARI allows...
Context. Starless cores represent a very early stage of the star formation process, before collapse...
International audienceContext. A solar-type system starts from an initial molecular core that acquir...
2.5-5 mu m spectra of four embedded protostars in the molecular core B35A were extracted using a nov...
2.5–5 μm spectra of four embedded protostars in the molecular core B35A were extracted using a novel...
We present near-infrared spectroscopic observations of 19 molecular clouds made using the AKARI sate...
34 pages, 9 figuresInternational audienceAbstract We present near-infrared spectra of three low-lumi...
To investigate the composition and evolution of circumstellar ice around low-mass young stellar obje...
Context. Circumstellar disks and envelopes of low-mass young stellar objects (YSOs) contain signific...
Circumstellar disks and envelopes of low-mass YSOs contain significant amounts of ice. Such icy mate...
Oral presentation given at the Terzo Workshop sull'Astronomia millimetrica e submillimetrica in Ital...
We present observations of L1155 and L1148 in the Cepheus molecular cloud, taken using the Far Infra...
Class 0 objects, which are thought to be the youngest protostars, are identified in terms of NIR or ...
The early stages of the formation of a planetary system are represented by Solar-type protostars. Re...
In dense cores, much of the molecular material is frozen on the surface of dust grains. AKARI allows...
Context. Starless cores represent a very early stage of the star formation process, before collapse...
International audienceContext. A solar-type system starts from an initial molecular core that acquir...