SDSS IV MaNGA – metallicity and nitrogen abundance gradients in local galaxies

By F. Belfiore, R. Maiolino, Christy A. Tremonti, S. S'anchez, K. Bundy, M. Bershady, K. Westfall, Lihwai Lin, N. Drory, M. Boquien and 2 more. 2017

185 citations recorded by the source corpus.

FB and RM acknowledge funding from the United Kingdom Science and Technology Facilities Council (STFC). RM acknowledges funding from the European Research Council (ERC), Advanced Grant 695671 ‘QUENCH’. SFS thanks the CONACYT- 125180, DGAPA-IA100815 and DGAPA-IA101217 projects for providing him support in this study. CAT acknowledges support from National Science Foundation of the United States grant 1412287 and 1554877. This work makes use of data from SDSS-IV. Funding for SDSS has been provided by the Alfred P. Sloan Foundation and Participating Institutions. Additional funding towards SDSS-IV has been provided by the U.S. Department of Energy Office of Science. SDSS-IV acknowledges support and resources from the Centre for High-Performance Computing at the University of Utah.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/5bb386ea09fb997c1860f65999c38d78d1e1d17b

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In Astronomy and Astrophysics

1. F. Mannucci
2. R. Maiolino
3. G. Cresci
4. M. Curti
5. P. Hopkins
6. M. Ouchi
7. R. Dav'e
8. K. Nakajima

Citations in the corpus

• The mass–metallicity and the fundamental metallicity relation revisited on a fully Te-based abundance scale for galaxies (2019, background): “, where they are generally steeper (Belfiore et al. 2017), which would make the central fibre-metallicity less representative of the global metallicity of the galaxy and therefore the comparison with the total SFR less fair.”