Laboratory astrophysics articles within Nature Communications

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  • Article
    | Open Access

    Probing molecules in excited vibrational states requires precise methods to extract the spectroscopic parameters. Here the authors demonstrate optical-optical double-resonance spectroscopy of excited-bands of methane using single pass high power continuous wave pump and cavity-enhanced frequency comb probe.

    • Vinicius Silva de Oliveira
    • , Isak Silander
    •  & Aleksandra Foltynowicz

  • Article
    | Open Access

    Nanobowls represent building blocks of fullerenes and nanotubes as detected in combustion systems and deep space, but their formation mechanisms in these environments have remained elusive. Here, the authors explore the gas-phase formation of benzocorannulene and beyond to the C40 nanobowl.

    • Lotefa B. Tuli
    • , Shane J. Goettl
    •  & Ralf I. Kaiser

  • Article
    | Open Access

    The abundances of small Polycyclic Aromatic Hydrocarbons (PAHs) observed in interstellar clouds has surprised astronomers and confounded astrochemical models. Here, the authors show that fast radiative cooling by Recurrent Fluorescence efficiently stabilizes the small PAH cation 1-cyanonaphthalene.

    • Mark H. Stockett
    • , James N. Bull
    •  & Boxing Zhu

  • Article
    | Open Access

    The triple-alpha process plays a role in nucleosynthesis, in the formation of 12C. Here, the authors discuss the rate and role of the neutron upscattering phenomenon on the triple-alpha process in a multi-step process.

    • J. Bishop
    • , C. E. Parker
    •  & C. Wheldon

  • Article
    | Open Access

    Ion storage rings allow reactions to be studied over orders of magnitude in time, bridging the gap between typical experimental and astronomical timescales. Here the authors observe that polycyclic aromatic hydrocarbon fragments produced upon collision with He atoms at velocities typical of stellar winds and supernova shockwaves remain intact up to second timescales, thus may play an important role in interstellar chemistry.

    • Michael Gatchell
    • , João Ameixa
    •  & Henning Zettergren

  • Article
    | Open Access

    Polycyclic aromatic hydrocarbons (PAHs) are present in the interstellar medium but their origin is unclear. Here the authors investigate large PAH formation from smaller PAHs in a plasma jet by mass-selective IR and UV laser spectroscopy, uncovering diacetylene radical addition as formation mechanism.

    • Alexander K. Lemmens
    • , Daniël B. Rap
    •  & Anouk M. Rijs

  • Article
    | Open Access

    The formation of nucleobases can take place in extraterrestrial environments. Here the authors show the simultaneous synthesis of three purine nucleobases and three pyrimidine from interstellar ice analogues that suggest the evolution from molecular clouds to stars and planets provide suitable environment for nucleobase synthesis in space.

    • Yasuhiro Oba
    • , Yoshinori Takano
    •  & Akira Kouchi

  • Article
    | Open Access

    Sugars are known to form from the UV photoprocessing of ices under astrophysical conditions. Here, the authors report the detection of deoxyribose, the sugar of DNA, and other deoxysugars from the UV photoprocessing of H2O:CH3OH ice mixtures, which are compared with materials from carbonaceous meteorites.

    • Michel Nuevo
    • , George Cooper
    •  & Scott A. Sandford

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