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The comet-like composition of a protoplanetary disk as revealed by complex cyanides

Author

Listed:
  • Karin I. Öberg

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA)

  • Viviana V. Guzmán

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA)

  • Kenji Furuya

    (Leiden Observatory, Leiden University, PO Box 9513, 2300 CA Leiden, The Netherlands)

  • Chunhua Qi

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA)

  • Yuri Aikawa

    (Kobe University, 1-1 Rokkodaicho, Nada Ward, Kobe, Hyogo Prefecture 657-0013, Japan)

  • Sean M. Andrews

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA)

  • Ryan Loomis

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA)

  • David J. Wilner

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA)

Abstract

The detection of complex cyanides in the protoplanetary disk around the young star MWC 480, and the similarity of their abundance ratios to those found in comets, implies that the rich organic chemistry of our solar nebula was not unique.

Suggested Citation

  • Karin I. Öberg & Viviana V. Guzmán & Kenji Furuya & Chunhua Qi & Yuri Aikawa & Sean M. Andrews & Ryan Loomis & David J. Wilner, 2015. "The comet-like composition of a protoplanetary disk as revealed by complex cyanides," Nature, Nature, vol. 520(7546), pages 198-201, April.
    • Handle: RePEc:nat:nature:v:520:y:2015:i:7546:d:10.1038_nature14276
    DOI: 10.1038/nature14276
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