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. Search

Refine search

Refine search

Access:
Content type:
Publication date:
Apply   From and To filters
Subject: Show more
Journals Show more
Publishers: Show more
Societies Show more
Series: Show more
Collections: Show more

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
×

1 results

  • 3D spectroscopy of Wolf-Rayet HII galaxies

  • C. Kehrig, E. Pérez-Montero, J. M. Vílchez, J. Brinchmann, D. Kunth, F. Durret, J. Iglesias-Páramo, J. Hernández-Fernández
  • Journal:
    Proceedings of the International Astronomical Union / Volume 10 / Issue S309 / July 2014
    Published online by Cambridge University Press:
    09 February 2015, pp. 155-156
    Print publication:
    July 2014
    • Article
      • You have access
    • PDF
    • Export citation

  • Wolf-Rayet HII galaxies are local metal-poor star-forming galaxies, observed when the most massive stars are evolving from O stars to WR stars, making them template systems to study distant starbursts. We have been performing a program to investigate the interplay between massive stars and gas in WR HII galaxies using IFS. Here, we highlight some results from the first 3D spectroscopic study of Mrk 178, the closest metal-poor WR HII galaxy, focusing on the origin of the nebular HeII emission and the aperture effects on the detection of WR features.