We observed ice absorption bands at NIR (2.5 μm–5.0 μm) towards field stars behind molecular clouds and low-mass YSOs with edge-on disk. We developed and tested a procedure to reduce the slitless spectroscopy data of extended object and the data with multiple objects in one field of view. Absorption bands of H2O, CO2 and CO are clearly detected towards field stars and YSOs. The spectral type and visual extinction of each field star are estimated using color-color diagram. The visual extinction of our field stars ranges from 15 mag to 25 mag. The column density of H2O ice towards our target stars ranges from 3×1017 cm-2 to 1×1019 cm-2, while the CO2 ice column density is (1–7)×1017 cm-2. These ice column densities are found to be roughly pro...
Molecular ices freeze out on the surface of dust grains within the interstellar medium (ISM). Dust g...
We have obtained 5-8 ${\rm \mu m }$ spectra towards 10 embedded protostars using the Short Wavelengt...
Apolar ices have been observed in several regions in dense clouds and are likely dominated by molecu...
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...
Context. Circumstellar disks and envelopes of low-mass young stellar objects (YSOs) contain signific...
We present new observations with the Infrared Spectrograph on board the Spitzer Space Telescope of t...
We present new observations with the Infrared Spectrograph on board the Spitzer Space Telescope of t...
A powerful way to observe directly the solid state inventory of dense molecular clouds is by infrare...
International audienceA powerful way to directly observe the solid-state inventory of dense molecula...
We present 2.5-30 mum spectra from the Short-Wavelength Spectrometer of the Infrared Space Observato...
We present 2.5-30 mum spectra from the Short-Wavelength Spectrometer of the Infrared Space Observato...
We present 2338È2322 cm~1 (4.277È4.307 km) infrared spectra of a number of mixedN2-containingmolecul...
We report the first detection of solid carbon dioxide (CO2) in quiescent regions of a dark cloud in ...
Spectra of interstellar CO2 ice absorption features at a resolving power of lambda/Delta lambda appr...
Molecular ices freeze out on the surface of dust grains within the interstellar medium (ISM). Dust g...
We have obtained 5-8 ${\rm \mu m }$ spectra towards 10 embedded protostars using the Short Wavelengt...
Apolar ices have been observed in several regions in dense clouds and are likely dominated by molecu...
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...
Context. Circumstellar disks and envelopes of low-mass young stellar objects (YSOs) contain signific...
We present new observations with the Infrared Spectrograph on board the Spitzer Space Telescope of t...
We present new observations with the Infrared Spectrograph on board the Spitzer Space Telescope of t...
A powerful way to observe directly the solid state inventory of dense molecular clouds is by infrare...
International audienceA powerful way to directly observe the solid-state inventory of dense molecula...
We present 2.5-30 mum spectra from the Short-Wavelength Spectrometer of the Infrared Space Observato...
We present 2.5-30 mum spectra from the Short-Wavelength Spectrometer of the Infrared Space Observato...
We present 2338È2322 cm~1 (4.277È4.307 km) infrared spectra of a number of mixedN2-containingmolecul...
We report the first detection of solid carbon dioxide (CO2) in quiescent regions of a dark cloud in ...
Spectra of interstellar CO2 ice absorption features at a resolving power of lambda/Delta lambda appr...
Molecular ices freeze out on the surface of dust grains within the interstellar medium (ISM). Dust g...
We have obtained 5-8 ${\rm \mu m }$ spectra towards 10 embedded protostars using the Short Wavelengt...
Apolar ices have been observed in several regions in dense clouds and are likely dominated by molecu...