Hostname: page-component-76fb5796d-22dnz Total loading time: 0 Render date: 2024-04-28T04:18:36.077Z Has data issue: false hasContentIssue false
  • English
  • Français

Star formation in the nuclear region of M83 The HST/NICMOS view

Published online by Cambridge University Press:  24 November 2004

T. Wiklind ,
A. Lundgren-Andersson  and
H. Olofsson
T. Wiklind
Affiliation:
ESA Space Telescope Division, STScI, 3700 San Martin Dr, Baltimore MD 21218, USA email: wiklind@stsci.edu
A. Lundgren-Andersson
Affiliation:
Stockholm Observatory, AlbaNova, SE-10691 Stockholm, Sweden European Southern Observatory, Casilla 19001, Santiago 19, Chile
H. Olofsson
Affiliation:
Stockholm Observatory, AlbaNova, SE-10691 Stockholm, Sweden
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The nuclear region of the barred spiral galaxy M83 has been imaged at near-infrared wavelengths with the HST NICMOS, showing a new region of star formation activity.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
POSTERS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 219 - 220
Copyright
© 2004 International Astronomical Union