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- Spanish National ObservatoryES106 papers
- Instituto de Física FundamentalES65 papers
- Centre National de la Recherche ScientifiqueFR52 papers
- Center for Astrophysics Harvard & SmithsonianUS34 papers
- Institut de Radioastronomie MillimétriqueFR32 papers
- Max Planck Institute for Radio AstronomyDE32 papers
- Chalmers University of TechnologySE30 papers
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- Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et AtmosphèresFR24 papers
7 papers · 2 filters
Gas-phase Elemental abundances in Molecular cloudS (GEMS) III. Unlocking the CS chemistry: the CS+O reaction
N. Bulut, O. Roncero, A. Aguado +36
CS is among the most abundant gas-phase S-bearing molecules in cold dark molecular clouds. It is easily observable with several transitions in the millimeter wavelength range, and…
Tentative detection of HC5NH+ in TMC-1
N. Marcelino, M. Agundez, B. Tercero +5
Using the Yebes 40m radio telescope, we report the detection of a series of seven lines harmonically related with a rotational constant B0=1295.81581 +/- 0.00026 MHz and a distorti…
Discovery of HC3O+ in space: The chemistry of O-bearing species in TMC-1
J. Cernicharo, N. Marcelino, M. Agundez +5
Using the Yebes 40m and IRAM 30m radio telescopes, we detected a series of harmonically related lines with a rotational constant B0=4460.590 +/- 0.001 MHz and a distortion constant…
Discovery of HC4NC in TMC-1: A study of the isomers of HC3N, HC5N, and HC7N
J. Cernicharo, N. Marcelino, M. Agundez +4
We present a study of the isocyano isomers of the cyanopolyynes HC3N, HC5N, and HC7N in TMC-1 and IRC+10216 carried out with the Yebes 40m radio telescope. This study has enabled u…
Interstellar nitrile anions: Detection of C3N- and C5N- in TMC-1
J. Cernicharo, N. Marcelino, J. R. Pardo +5
We report on the first detection of C3N- and C5N- towards the cold dark core TMC-1 in the Taurus region, using the Yebes 40 m telescope. The observed C3N/C3N- and C5N/C5N- abundanc…
Cloud-cloud collision as drivers of the chemical complexity in Galactic Centre molecular clouds
S. Zeng, Q. Zhang, I. Jimenez-Serra +6
G+0.693-0.03 is a quiescent molecular cloud located within the Sagittarius B2 (Sgr B2) star-forming complex. Recent spectral surveys have shown that it represents one of the most p…