Planetary nebula carbon yields and the chemical evolution of the Galactic disc
Open Access
- 1 March 2003
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 339 (3) , 825-833
- https://doi.org/10.1046/j.1365-8711.2003.06225.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 21 references indexed in Scilit:
- A Reappraisal of the Solar Photospheric C/O RatioThe Astrophysical Journal, 2002
- Galactic chemical abundance evolution in the solar neighborhood up to the iron peakAstronomy & Astrophysics, 2001
- The Chemical Evolution of the Galaxy with Variable Initial Mass FunctionsThe Astrophysical Journal, 2000
- Dark Matter and the Chemical Evolution of Irregular GalaxiesThe Astrophysical Journal, 1999
- Carbon in Spiral Galaxies fromHubble Space TelescopeSpectroscopyThe Astrophysical Journal, 1999
- Faint Emission Lines and Temperature Fluctuations in M8The Astrophysical Journal Supplement Series, 1999
- Chemical composition of the Orion nebula derived from echelle spectrophotometryMonthly Notices of the Royal Astronomical Society, 1998
- The Chemical Evolution of the Galaxy: The Two‐Infall ModelThe Astrophysical Journal, 1997
- Chemical evolution of irregular and blue compact galaxiesThe Astrophysical Journal, 1995
- The unique planetary nebula NGC 2818The Astrophysical Journal, 1984