Interstellar abundances in the neutral and ionized gas of NGC 604

2006/08/21 by V. Lebouteiller, D. Kunth, J. Lequeux +10 · 20 citations
Physics and Astronomy · #Absorption spectroscopy #Abundance (ecology) #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Emission spectrum #Galaxies: Formation, Evolution, Phenomena #Galaxy #Interstellar medium #Ion #Ionization #Optics #Physics #Spectral line #Spiral galaxy #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20053161

published in Astronomy and Astrophysics 459(1), 161-174 (EDP Sciences) · Accepted for publication in A&A

arxiv created 2006/08/21 · openalex publication_date 2006/08/25 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims.We present FUSE spectra of the giant H ii region NGC 604 in the spiral galaxy M 33. Chemical abundances are tentatively derived from far-UV absorption lines and compared to those derived from optical emission lines.

Citations

• CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra

Cited by

• TheChandraACIS Survey of M33 (ChASeM33): Investigating the Hot Ionized Medium in NGC 604
• Metal enrichment of the neutral gas of blue compact dwarf galaxies: the compelling case of Pox 36