Episodic molecular outflow in the very young protostellar cluster Serpens South

Adele L. Plunkett (), Héctor G. Arce (), Diego Mardones, Pieter van Dokkum, Michael M. Dunham, Manuel Fernández-López, José Gallardo and Stuartt A. Corder
Additional contact information
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

Nature, 2015, vol. 527, issue 7576, 70-73

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.

Date: 2015
References: Add references at CitEc
Citations:

Downloads: (external link)
https://www.nature.com/articles/nature15702 Abstract (text/html)
Access to the full text of the articles in this series is restricted.

Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.

Export reference: BibTeX RIS (EndNote, ProCite, RefMan) HTML/Text

Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:527:y:2015:i:7576:d:10.1038_nature15702

Ordering information: This journal article can be ordered from
https://www.nature.com/

DOI: 10.1038/nature15702

Access Statistics for this article

Nature is currently edited by Magdalena Skipper

More articles in Nature from Nature
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().