Skip to main content Accessibility help

We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.

Close cookie message
×
  1. Home
  2. Journals
  3. Proceedings of the International Astronomical Union
  4. Volume 6 Issue s275: jets at all scales
Journal Home
Refine listing

Refine listing

Access:
Publication date:

Actions for selected content:

Select all | Deselect all
  • View selected items
  • Export citations
  • Download PDF (zip)
  • Save to Kindle
  • Save to Dropbox
  • Save to Google Drive

Save Search

You can save your searches here and later view and run them again in "My saved searches".

Please provide a title, maximum of 40 characters.
Cancel
×

Jets at all Scales

Volume 6 - Issue S275 - September 2010
Contents

Page 6 of 6

Contributed Papers

  • What is shaping the planetary nebula K3-35?

  • Y. Gómez, D. Tafoya, G. Anglada, L. F. Miranda, L. Uscanga, J. M. Torrelles, P. F. Velázquez
  • Published online by Cambridge University Press:
    24 February 2011, pp. 414-415
    • Article
      • You have access
    • PDF
    • Export citation
    • NASA ADS Abstract Service

  • K 3-35 is a very young planetary nebula (PN) with a characteristic S-shaped radio emission morphology. It is the first PN where water vapor maser was detected: the emission is located in a torus-like structure with a radius of 100 AU and also at the surprisingly large distance of 5000 AU from the star, in the tips of the bipolar lobes. Several mechanism have been proposed to explain the bipolar morphology of PNe, and in the case of K 3-35 we believe we may be observing several of them at the same time: i) a disk-like structure traced by the H2O masers, ii) a precessing bipolar jet probably due to the presence of a binary companion and iii) circular polarization in the OH 1665 MHz masers, which suggests the presence of a magnetic field. Additional observations and modeling are needed to establish what mechanisms are shaping K 3-35.

Front Cover and matter

  • IAU volume 6 issue S275 Cover and Front matter

  • Published online by Cambridge University Press:
    24 February 2011, pp. f1-f19
    • Article
      • You have access
    • PDF
    • Export citation
    • NASA ADS Abstract Service

Back Cover and matter

  • IAU volume 6 issue S275 Cover and Back matter

  • Published online by Cambridge University Press:
    24 February 2011, pp. b1-b8
    • Article
      • You have access
    • PDF
    • Export citation
    • NASA ADS Abstract Service

Page 6 of 6