Galaxy And Mass Assembly (GAMA): the interplay between galaxy mass, SFR, and heavy element abundance in paired galaxy sets

Authors

L. E. Garduno, Instituto Nacional de Astrofısica
M. A. Lara-Lopez, Niels Bohr Institute
O. Lopez-Cruz, Instituto Nacional de Astrofısica
A. M. Hopkins, Australian Astronomical Observatory
M. S. Owers, Macquarie University
K. A. Pimbblet, University of Hull
Benne Holwerda, University of LouisvilleFollow

Document Type

Article

Publication Date

2021

Department

Physics and Astronomy

Abstract

We study the star formation rate (SFR), stellar mass (M), and the gas metallicity (Z) for 4636 galaxy pairs using the Galaxy And Mass Assembly (GAMA) survey. Our galaxy pairs lie in a redshift range of 0

Comments

C 2020 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. MNRAS 501, 2969–2982 (2021).

ThinkIR Citation

Garduno, L. E.; Lara-Lopez, M. A.; Lopez-Cruz, O.; Hopkins, A. M.; Owers, M. S.; Pimbblet, K. A.; and Holwerda, Benne, "Galaxy And Mass Assembly (GAMA): the interplay between galaxy mass, SFR, and heavy element abundance in paired galaxy sets" (2021). Faculty and Staff Scholarship. 467.
https://ir.library.louisville.edu/faculty/467

DOI

10.1093/mnras/staa3799

ORCID

0000-0002-4884-6756