Contains fulltext : 149321.pdf (publisher's version ) (Open Access
Determining the level of chemical complexity within dense starless and gravitationally bound pre-ste...
Context. Formic acid (HCOOH) and carbon dioxide (CO2) are simple species that have been detected in ...
International audienceContext. Hydrides are simple compounds containing one or a few hydrogen atoms ...
The prominent infrared absorption band of solid CO – commonly observed towards young stellar objects...
textWe present observations toward stars behind molecular clouds (back ground stars) and toward mas...
Data from observations of star forming regions and laboratory surface-astrochemistry experiments hav...
The formation of CH+ in the interstellar medium (ISM) has long been an outstanding problem in chemic...
Context. The molecular composition of interstellar ice mantles is defined by gas-grain processes in ...
Investigating the elusive relationship between our interstellar medium and its assortment of complex...
[Context] Hydrides are simple compounds containing one or a few hydrogen atoms bonded to a heavier a...
The formation of complex organic molecules that consist of more than four atoms in space is one of t...
Context. The chemistry of the diffuse interstellar medium is driven by the combined influences of co...
Author Institution: Department of Chemistry, Department of Astronomy, Arizona Radio Observatory, and...
Author Institution: Herzberg Institute of Astrophysics, National Research Council of CanadaFormaldeh...
International audienceHydrides are simple compounds containing one or a few hydrogen atoms bonded to...
Determining the level of chemical complexity within dense starless and gravitationally bound pre-ste...
Context. Formic acid (HCOOH) and carbon dioxide (CO2) are simple species that have been detected in ...
International audienceContext. Hydrides are simple compounds containing one or a few hydrogen atoms ...
The prominent infrared absorption band of solid CO – commonly observed towards young stellar objects...
textWe present observations toward stars behind molecular clouds (back ground stars) and toward mas...
Data from observations of star forming regions and laboratory surface-astrochemistry experiments hav...
The formation of CH+ in the interstellar medium (ISM) has long been an outstanding problem in chemic...
Context. The molecular composition of interstellar ice mantles is defined by gas-grain processes in ...
Investigating the elusive relationship between our interstellar medium and its assortment of complex...
[Context] Hydrides are simple compounds containing one or a few hydrogen atoms bonded to a heavier a...
The formation of complex organic molecules that consist of more than four atoms in space is one of t...
Context. The chemistry of the diffuse interstellar medium is driven by the combined influences of co...
Author Institution: Department of Chemistry, Department of Astronomy, Arizona Radio Observatory, and...
Author Institution: Herzberg Institute of Astrophysics, National Research Council of CanadaFormaldeh...
International audienceHydrides are simple compounds containing one or a few hydrogen atoms bonded to...
Determining the level of chemical complexity within dense starless and gravitationally bound pre-ste...
Context. Formic acid (HCOOH) and carbon dioxide (CO2) are simple species that have been detected in ...
International audienceContext. Hydrides are simple compounds containing one or a few hydrogen atoms ...