The gas-phase metallicities of star-forming galaxies in aperture-matched SDSS samples follow potential rather than mass or average surface density-Reference-Cited by-同舟云学术

The gas-phase metallicities of star-forming galaxies in aperture-matched SDSS samples follow potential rather than mass or average surface density

Author:

D’Eugenio Francesco¹²³,Colless Matthew¹²⁴^ORCID,Groves Brent¹⁴,Bian Fuyan¹,Barone Tania M¹²⁴⁵

Affiliation:

1. Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia

2. Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO)

3. Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281 S9, B-9000 Gent, Belgium

4. ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia

5. Sydney Institute for Astronomy, School of Physics, The University of Sydney, NSW 2006, Australia

Funder

Australian Research Council Centre of Excellence for All-sky Astrophysics

Australian Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference87 articles.

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2. A tight N/O–potential relation in star-forming galaxies;Monthly Notices of the Royal Astronomical Society: Letters;2024-07-27