The bends in the slopes of radial abundance gradients in the disks of spiral galaxies – Do they exist?
Open Access
- 11 December 2002
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 397 (1) , 109-114
- https://doi.org/10.1051/0004-6361:20021505
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsKeywords
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This publication has 26 references indexed in Scilit:
- A comprehensive study of reported high-metallicity giant H ii regions — I. Detailed abundance analysisMonthly Notices of the Royal Astronomical Society, 2002
- The Hazards of Imaging Spectrophotometry with Interference FiltersThe Astronomical Journal, 2001
- Carbon in Spiral Galaxies fromHubble Space TelescopeSpectroscopyThe Astrophysical Journal, 1999
- Interstellar Abundance Gradients In NGC 2403: Comparison To M33The Astrophysical Journal, 1997
- The form of abundance gradients in three nearby spiral galaxies: M33, M81 and M101The Astrophysical Journal, 1995
- On the influence of bars and star formation on galactic abundance gradientsThe Astrophysical Journal, 1994
- A very metal poor H II region in the outer disk of M101The Astrophysical Journal, 1994
- Third Reference Catalogue of Bright GalaxiesPublished by Springer Nature ,1991
- Chemical composition gradient in NGC 2403 and the stellar mass limitPublications of the Astronomical Society of the Pacific, 1986
- On the composition of H II regions in southern galaxies - III. NGC 2997 and 7793Monthly Notices of the Royal Astronomical Society, 1984