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  • Surcis, G.Joint Institute for VLBI in Europe (JIVE) (författare)

Rapidly increasing collimation and magnetic field changes of a protostellar H2O maser outflow

  • Artikel/kapitelEngelska2014

Förlag, utgivningsår, omfång ...

  • 2014-05-22
  • EDP Sciences,2014
  • electronicrdacarrier

Nummerbeteckningar

  • LIBRIS-ID:oai:research.chalmers.se:bdc05e44-f504-480a-9510-540055aad514
  • https://research.chalmers.se/publication/200317URI
  • https://doi.org/10.1051/0004-6361/201423877DOI

Kompletterande språkuppgifter

  • Språk:engelska
  • Sammanfattning på:engelska

Ingår i deldatabas

Klassifikation

  • Ämneskategori:art swepub-publicationtype
  • Ämneskategori:ref swepub-contenttype

Anmärkningar

  • Context. W75N(B) is a massive star-forming region that contains three radio continuum sources (VLA 1, VLA 2, and VLA 3), which are thought to be three massive young stellar objects at three different evolutionary stages. VLA 1 is the most evolved and VLA 2 the least evolved source. The 22 GHz H2O masers associated with VLA 1 and VLA 2 have been mapped at several epochs over eight years. While the H2O masers in VLA 1 show a persistent linear distribution along a radio jet, those in VLA 2 are distributed around an expanding shell. Furthermore, H2O maser polarimetric measurements revealed magnetic fields aligned with the two structures. Aims. Using new polarimetric observations of H2O masers, we aim to confirm the elliptical expansion of the shell-like structure around VLA 2 and, at the same time, to determine if the magnetic fields around the two sources have changed. Methods. The NRAO Very Long Baseline Array was used to measure the linear polarization and the Zeeman-splitting of the 22 GHz H2O masers towards the massive star-forming region W75N(B). Results. The H2O maser distribution around VLA 1 is unchanged from that previously observed. We made an elliptical fit of the H2O masers around VLA 2. We find that the shell-like structure is still expanding along the direction parallel to the thermal radio jet of VLA 1. While the magnetic field around VLA 1 has not changed in the past similar to 7 years, the magnetic field around VLA 2 has changed its orientation according to the new direction of the major-axis of the shell-like structure and it is now aligned with the magnetic field in VLA 1.

Ämnesord och genrebeteckningar

Biuppslag (personer, institutioner, konferenser, titlar ...)

  • Vlemmings, Wouter,1974Chalmers tekniska högskola,Chalmers University of Technology(Swepub:cth)wouterv (författare)
  • van Langevelde, H. J.Universiteit Leiden (UL),Leiden University (UL),Joint Institute for VLBI in Europe (JIVE) (författare)
  • Goddi, C.Joint Institute for VLBI in Europe (JIVE) (författare)
  • Torrelles, J. M.Institut de Ciències de l'Espai (ICE) - CSIC,Institute of Space Sciences (ICE) - CSIC (författare)
  • Canto, J.Universidad Nacional Autónoma de México (UNAM),Universidad Nacional Autonoma de Mexico (författare)
  • Curiel, S.Universidad Nacional Autónoma de México (UNAM),Universidad Nacional Autonoma de Mexico (författare)
  • Kim, S. W.Korea Astronomy and Space Science Institute (författare)
  • Kim, J. S.National Astronomical Observatory of Japan (författare)
  • Joint Institute for VLBI in Europe (JIVE)Chalmers tekniska högskola (creator_code:org_t)

Sammanhörande titlar

  • Ingår i:Astronomy and Astrophysics: EDP Sciences5650004-63611432-0746

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