Aims.We study the chemical origin of a set of complex organic molecules thought to be produced by grain surface chemistry in high mass young stellar objects (YSOs). Methods.A partial submillimeter line-survey was performed toward 7 high-mass YSOs aimed at detecting H2CO, CH3OH, CH2CO, CH3CHO, C2H5OH, HCOOH, HNCO and NH2CHO. In addition, lines of CH3CN, C2H5CN, CH3CCH, HCOOCH3, and CH3OCH3 were observed. Rotation temperatures and beam-averaged column densities are determined. To correct for beam dilution and determine abundances for hot gas, the radius and H2 column densities of gas at temperatures >100 K are computed using 850 μm dust continuum data and source luminosity. Results.Based on their rotation diagrams, molecules c...
International audienceWe investigate the presence of complex organic molecules (COMs) in strongly UV...
We present the results ofa line identification analysis using data from theIRAMPlateau de Bure Plate...
Aims.We have observed several emission lines of two Nitrogen-bearing (C2H5CN and C2H3CN) and two O...
Aims.We study the chemical origin of a set of complex organic molecules thought to be produced by gr...
Context. Massive young stellar objects (MYSOs) with hot cores are classic sources of complex organic...
Aims. Our goal is to take an inventory of complex molecules in three well-known high-mass protostars...
Context. The presence of many interstellar complex organic molecules (COMs) in the gas phase in the ...
The different distributions of N-bearing species and O-bearing species, as is well known towards Ori...
International audienceContext. The recent unexpected detection of terrestrial complex organic molecu...
Interstellar complex organic molecules were first identified in the hot inner regions of massive you...
Context. The recent unexpected detection of terrestrial complex organic molecules in the cold (~10 K...
Context. The presence of many interstellar complex organic molecules (COMs) in the gas phase in the ...
Recent astrochemical models and experiments have explained that complex organic molecules (COMs; mol...
Complex molecules have been broadly classified into three generations dependent on the mode of forma...
Author Institution: Emory University, Department of Chemistry, Atlanta, Georgia 30322Advancements in...
International audienceWe investigate the presence of complex organic molecules (COMs) in strongly UV...
We present the results ofa line identification analysis using data from theIRAMPlateau de Bure Plate...
Aims.We have observed several emission lines of two Nitrogen-bearing (C2H5CN and C2H3CN) and two O...
Aims.We study the chemical origin of a set of complex organic molecules thought to be produced by gr...
Context. Massive young stellar objects (MYSOs) with hot cores are classic sources of complex organic...
Aims. Our goal is to take an inventory of complex molecules in three well-known high-mass protostars...
Context. The presence of many interstellar complex organic molecules (COMs) in the gas phase in the ...
The different distributions of N-bearing species and O-bearing species, as is well known towards Ori...
International audienceContext. The recent unexpected detection of terrestrial complex organic molecu...
Interstellar complex organic molecules were first identified in the hot inner regions of massive you...
Context. The recent unexpected detection of terrestrial complex organic molecules in the cold (~10 K...
Context. The presence of many interstellar complex organic molecules (COMs) in the gas phase in the ...
Recent astrochemical models and experiments have explained that complex organic molecules (COMs; mol...
Complex molecules have been broadly classified into three generations dependent on the mode of forma...
Author Institution: Emory University, Department of Chemistry, Atlanta, Georgia 30322Advancements in...
International audienceWe investigate the presence of complex organic molecules (COMs) in strongly UV...
We present the results ofa line identification analysis using data from theIRAMPlateau de Bure Plate...
Aims.We have observed several emission lines of two Nitrogen-bearing (C2H5CN and C2H3CN) and two O...