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Astronomy and astrophysics (Berlin), ISSN 0004-6361, 03/2014, Volume 563, pp. A33 - np
.... Small, simple molecules have traditionally been detected in protoplanetary disks; however, in the ALMA era, we expect the molecular inventory of protoplanetary disks to significantly increase. Aims... 
Astrochemistry | Protoplanetary disks | ISM: molecules | Stars: formation | Physical Sciences | Astronomy & Astrophysics | Science & Technology | COM | Protoplanets | Planet formation | Stars | T Tauri stars | Mathematical models | Density | Planetary systems
Journal Article
Monthly notices of the Royal Astronomical Society. Letters, ISSN 1745-3925, 02/2015, Volume 449, Issue 1, pp. L16 - L20
While astrochemical models are successful in reproducing many of the observed interstellar species, they have been struggling to explain the observed abundances of complex organic molecules... 
ISM: molecules | ISM: abundances | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics - Solar and Stellar Astrophysics
Journal Article
Astrophysical journal. Letters, ISSN 2041-8205, 11/2014, Volume 795, Issue 1, pp. L2 - 6
Journal Article
The Astrophysical journal, ISSN 1538-4357, 02/2018, Volume 854, Issue 2, p. 116
...). The spectral line profile of CH3CHO is found to reveal a well-separated double peak. It is similar to the line profile of CH3OH, but is much different from those of carbon-chain molecules and (CS)-S-34... 
ISM: molecules | ISM: abundances | ISM: individual objects (TMC-1) | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Organic chemistry | Molecular clouds | Biological evolution | Rotational spectra | Millimeter waves | Chains | Line spectra | Carbon
Journal Article
Journal Article
The Astrophysical Journal Letters, ISSN 2041-8205, 06/2011, Volume 733, Issue 2, p. L36
Journal Article
The Astrophysical journal, ISSN 1538-4357, 07/2014, Volume 791, Issue 1, pp. 29 - 6
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2012, Volume 538, p. A2
.... Reproducing these counterparts is an important new challenge for proposed ejection models. Aims. We explore whether molecules may survive in the magneto-hydrodynamic... 
stars: mass-loss | stars: formation | ISM: jets and outflows | accretion, accretion disks | ISM: molecules | astrochemistry | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics - Solar and Stellar Astrophysics | Galactic Astrophysics | Sciences of the Universe | Astrophysics | Physics
Journal Article