Multiwavelength analysis of active star forming regions: The case of NGC 604

DOI: 
10.1023/A:1012711424646
Publication date: 
01/01/2001
Main author: 
González Delgado, Rosa M.
IAA authors: 
González Delgado, Rosa M.;Pérez, Enrique
Authors: 
González Delgado, Rosa M.;Pérez, Enrique
Journal: 
Astrophysics and Space Science Supplement
Publication type: 
Article
Volume: 
277
Pages: 
259-262
Abstract: 
We analyse the integrated ultraviolet and optical spectra of the active star forming region NGC 604. The ultraviolet resonance wind stellar lines, the nebular optical emission lines and the higher order terms of the Balmer series and HeI absorption lines detected are interpreted using evolutionary models optimized for young star forming regions. The evolutionary state and the massive stellar content of the region is derived in a self-consistent way.
Database: 
ADS
URL: 
https://ui.adsabs.harvard.edu/#abs/2001ApSSS.277..259G/abstract
ADS Bibcode: 
2001ApSSS.277..259G
Keywords: 
GALAXIES: EVOLUTION;GALAXIES: STELLAR CONTENT;ISM: HII REGIONS