Advanced search

Filter By:

Journal Check one or more journals to show results from those journals only.

Choose more journals

Article type Check one or more article types to show results from those article types only.
Subject Check one or more subjects to show results from those subjects only.
Date Choose a date option to show results from those dates only.

Custom date range

Clear all filters
Sort by:
Showing 1–5 of 5 results
Advanced filters: Author: Christine Joblin Clear advanced filters

  • Using an atomic gas aggregation process in the laboratory to simulate the conditions in the inner regions of a carbon-rich evolved star, Martínez, Santoro, Merino and colleagues. show that aromatic species and fullerenes form surprisingly inefficiently, and that amorphous carbon nanograins and aliphatic clusters dominate.

    • Lidia Martínez
    • Gonzalo Santoro
    • José A. Martín-Gago
    Research
    Nature Astronomy
    Volume: 4, P: 97-105

  • JWST reveals the chemistry of the disk of a young star in the Orion nebula, showing that it has water and CO in its inner regions that are shielded from UV radiation, whereas UV-processed molecules such as CH3+ and PAHs are detected in surface layers.

    • Ilane Schroetter
    • Olivier Berné
    • Marion Zannese
    Research
    Nature Astronomy
    Volume: 9, P: 1326-1336

  • The hydroxyl radical OH has been detected in a planet-forming disk exposed to ultraviolet radiation and in a rovibrationally excited state. These JWST observations, when coupled with quantum calculations, reveal the ongoing photodissociation of water and its reformation in the gas phase.

    • Marion Zannese
    • Benoît Tabone
    • Mark G. Wolfire
    Research
    Nature Astronomy
    Volume: 8, P: 577-586

  • JWST observations of CH3+ in a protoplanetary disk in the Orion star-forming region are reported showing that gas-phase organic chemistry in the interstellar medium is activated by ultraviolet irradiation and the methyl cation.

    • Olivier Berné
    • Marie-Aline Martin-Drumel
    • Mark G. Wolfire
    Research
    Nature
    Volume: 621, P: 56-59

  • One-arcsecond-resolution millimetre-wave images enable the surface of the Orion Bar molecular cloud to be resolved, revealing a fragmented ridge of high-density substructures, photoablative gas flows and instabilities that suggest that the cloud edge has been compressed by a high-pressure wave expanding into the molecular cloud, in contrast to predictions from static equilibrium models.

    • Javier R. Goicoechea
    • Jérôme Pety
    • Paolo Pilleri
    Research
    Nature
    Volume: 537, P: 207-209