Abundances in HII regions and PNe of M81

DOI

M81 is an ideal laboratory to investigate the galactic chemical and dynamical evolution through the study of its young and old stellar populations. We analyze the chemical abundances of planetary nebulae and HII regions in the M81 disk for insight on galactic evolution, and compare it with that of other galaxies, including the Milky Way.

Cone search capability for table J/A+A/521/A3/table1 (Observing log)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35210003
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/521/A3
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/521/A3
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/521/A3
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/521/A3
Provenance
Creator Stanghellini L.; Magrini L.; Villaver E.; Galli D.
Publisher CDS
Publication Year 2010
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Interdisciplinary Astronomy; Interstellar medium; Natural Sciences; Physics