Observing the onset of outflow collimation in a massive protostar
Artikel i vetenskaplig tidskrift, 2015

The current paradigm of star formation through accretion disks, and magnetohydrodynamically driven gas ejections, predicts the development of collimated outflows, rather than expansion without any preferential direction. We present radio continuum observations of the massive protostar W75N(B)-VLA 2, showing that it is a thermal, collimated ionized wind and that it has evolved in 18 years from a compact source into an elongated one. This is consistent with the evolution of the associated expanding water-vapor maser shell, which changed from a nearly circular morphology, tracing an almost isotropic outflow, to an elliptical one outlining collimated motions. We model this behavior in terms of an episodic, short-lived, originally isotropic ionized wind whose morphology evolves as it moves within a toroidal density stratification.


C. Carrasco-Gonzalez

Universidad Nacional Autonoma de Mexico

J. M. Torrelles

Institut de Ciències de l'Espai (ICE) - CSIC

J. Canto

Universidad Nacional Autonoma de Mexico

S. Curiel

Universidad Nacional Autonoma de Mexico

G. Surcis

Joint Institute for VLBI in Europe (JIVE)

Wouter Vlemmings

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

H. J. van Langevelde

Joint Institute for VLBI in Europe (JIVE)

Universiteit Leiden

C. Goddi

Joint Institute for VLBI in Europe (JIVE)

Radboud Universiteit

G. Anglada

Instituto de Astrofisica de Andalucía (IAA)

S. W. Kim

University of Science and Technology (UST)

Korea Astronomy and Space Science Institute

J. S. Kim

National Astronomical Observatory of Japan

J. F. Gomez

Instituto de Astrofisica de Andalucía (IAA)


0036-8075 (ISSN)

Vol. 348 6230 114-117

Magnetic fields and the outflows during the formation and evolution of stars (OUTFLOWMAGN)

Europeiska kommissionen (EU), 2014-05-01 -- 2019-04-30.


Astronomi, astrofysik och kosmologi


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