- Centre National de la Recherche ScientifiqueFR2.7k papers
- Laboratoire d'Astrophysique de BordeauxFR1k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR557 papers
- Institut de Mathématiques de BordeauxFR410 papers
- Laboratoire Bordelais de Recherche en InformatiqueFR390 papers
- Laboratoire Ondes et Matière d'AquitaineFR347 papers
- Institut Polytechnique de BordeauxFR314 papers
- Laboratoire de Physique des deux infinis BordeauxFR314 papers
- Sorbonne UniversitéFR312 papers
- CEA Paris-SaclayFR309 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR299 papers
- Astrophysique, Instrumentation et ModélisationFR278 papers
27 papers · 2 filters
Observations of water with Herschel/HIFI toward the high-mass protostar AFGL 2591
Y. Choi, F. F. S. van der Tak, E. F. van Dishoeck +2
Water is a sensitive tracer of physical conditions in star-forming regions because of its large abundance variations between hot and cold regions. We use spectrally resolved observ…
The Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO)
R. Carrera, L. Casamiquela, L. Balaguer-Núñez +10
We present the motivation, design and current status of the Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO). Using the high resolution spectroscopic fac…
New N-bearing species towards OH231.8+4.2: HNCO, HNCS, HCN and NO
L. Velilla Prieto, C. Sánchez Contreras, J. Cernicharo +7
OH231.8+4.2 is a well studied O-rich CSE around an intermediate-mass evolved star that displays bipolar molecular outflows accelerated up to 400 km/s. OH231 also presents an except…
Chemical modeling of water deuteration in IRAS16293-2422
V. Wakelam, C. Vastel, Y. Aikawa +3
IRAS 16293-2422 is a well studied low-mass protostar characterized by a strong level of deuterium fractionation. In the line of sight of the protostellar envelope, an additional ab…
13C-methyl formate: observations of a sample of high mass star-forming regions including Orion-KL and spectroscopic characterization
Cecile Favre, Miguel Carvajal, David Field +12
We have surveyed a sample of massive star-forming regions located over a range of distances from the Galactic centre for methyl formate, HCOOCH, and its isotopologues H$^{13}…
Revised spectroscopic parameters of SH from ALMA and IRAM 30 m observations
Holger S. P. Müller, Javier R. Goicoechea, José Cernicharo +6
Hydrides represent the first steps of interstellar chemistry. Sulfanylium (SH), in particular, is a key tracer of energetic processes. We used ALMA and the IRAM 30 m telescope…