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Gas flow and accretion via spiral streamers and circumstellar disks in a young binary protostar

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Science  04 Oct 2019:
Vol. 366, Issue 6461, pp. 90-93
DOI: 10.1126/science.aaw3491

Article Information

vol. 366 no. 6461 90-93

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History: 
  • Received for publication December 17, 2018
  • Accepted for publication September 9, 2019
  • .

Author Information

  1. F. O. Alves1,*,
  2. P. Caselli1,
  3. J. M. Girart2,3,
  4. D. Segura-Cox1,
  5. G. A. P. Franco4,
  6. A. Schmiedeke1,
  7. B. Zhao1
  1. 1Center for Astrochemical Studies, Max Planck Institute for Extraterrestrial Physics, Garching, 85748, Germany.
  2. 2Institut de Ciències de l’Espai, Consejo Superior de Investigaciones Científicas, Cerdanyola del Vallès, E-08193, Catalunya, Spain.
  3. 3Institut d’Estudis Espacials de Catalunya, Barcelona, E-08034, Spain.
  4. 4Departamento de Física, Instituto de Ciências Exatas, Universidade Federal de Minas Gerais, Belo Horizonte, 30.123-970, Brazil.
  1. *Corresponding author. Email: falves{at}mpe.mpg.de

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