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Episodic molecular outflow in the very young protostellar cluster Serpens South

Author

Listed:
  • Adele L. Plunkett

    (Yale University)

  • Héctor G. Arce

    (Yale University)

  • Diego Mardones

    (Universidad de Chile)

  • Pieter van Dokkum

    (Yale University)

  • Michael M. Dunham

    (Harvard-Smithsonian Center for Astrophysics)

  • Manuel Fernández-López

    (Instituto Argentino de Radioastronomía, CCT-La Plata (CONICET))

  • José Gallardo

    (Joint ALMA Observatory)

  • Stuartt A. Corder

    (Joint ALMA Observatory)

Abstract

A study of 12CO outflow emission from the protostellar source CARMA-7 in the cluster Serpens South suggests that episodic ejections of mass by the protostar begin in the earliest phase of protostellar evolution, probably providing a mechanism for driving the turbulence that is necessary for star formation in clusters.

Suggested Citation

  • Adele L. Plunkett & Héctor G. Arce & Diego Mardones & Pieter van Dokkum & Michael M. Dunham & Manuel Fernández-López & José Gallardo & Stuartt A. Corder, 2015. "Episodic molecular outflow in the very young protostellar cluster Serpens South," Nature, Nature, vol. 527(7576), pages 70-73, November.
    • Handle: RePEc:nat:nature:v:527:y:2015:i:7576:d:10.1038_nature15702
    DOI: 10.1038/nature15702
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