Abundances in HII regions and PNe of M81 Virtual Observatory Resource

Authors

1. Stanghellini L.
2. Magrini L.
3. Villaver E.
4. Galli D.

Published by

CDS

Abstract

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.

Keywords

1. galaxies
2. h-ii-regions
3. planetary-nebulae
4. chemical-abundances

Bibliographic source Bibcode

2010A&A...521A...3S

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/521/A3

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/521/A3

Document Object Identifer DOI

doi:10.26093/cds/vizier.35210003

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/521/A3
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/521/A3
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/521/A3

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/521/A3/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/521/A3/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/521/A3/table1?