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Galaxy And Mass Assembly (GAMA) : the interplay between galaxy mass, SFR, and heavy element abundance in paired galaxy sets. / Garduno, L. E.; Lara-Lopez, M. A.; Lopez-Cruz, O.; Hopkins, A. M.; Owers, M. S.; Pimbblet, K. A.; Holwerda, B. W.
In:
Monthly Notices of the Royal Astronomical Society, Vol. 501, No. 2, 01.02.2021, p. 2969-2982.
Research output: Contribution to journal › Journal article › Research › peer-review
Harvard
Garduno, LE, Lara-Lopez, MA, Lopez-Cruz, O, Hopkins, AM, Owers, MS, Pimbblet, KA & Holwerda, BW 2021, '
Galaxy And Mass Assembly (GAMA): the interplay between galaxy mass, SFR, and heavy element abundance in paired galaxy sets',
Monthly Notices of the Royal Astronomical Society, vol. 501, no. 2, pp. 2969-2982.
https://doi.org/10.1093/mnras/staa3799APA
Garduno, L. E., Lara-Lopez, M. A., Lopez-Cruz, O., Hopkins, A. M., Owers, M. S., Pimbblet, K. A., & Holwerda, B. W. (2021).
Galaxy And Mass Assembly (GAMA): the interplay between galaxy mass, SFR, and heavy element abundance in paired galaxy sets.
Monthly Notices of the Royal Astronomical Society,
501(2), 2969-2982.
https://doi.org/10.1093/mnras/staa3799Vancouver
Garduno LE, Lara-Lopez MA, Lopez-Cruz O, Hopkins AM, Owers MS, Pimbblet KA et al.
Galaxy And Mass Assembly (GAMA): the interplay between galaxy mass, SFR, and heavy element abundance in paired galaxy sets.
Monthly Notices of the Royal Astronomical Society. 2021 Feb 1;501(2):2969-2982.
https://doi.org/10.1093/mnras/staa3799Author
Garduno, L. E. ; Lara-Lopez, M. A. ; Lopez-Cruz, O. ; Hopkins, A. M. ; Owers, M. S. ; Pimbblet, K. A. ; Holwerda, B. W. / Galaxy And Mass Assembly (GAMA) : the interplay between galaxy mass, SFR, and heavy element abundance in paired galaxy sets. In: Monthly Notices of the Royal Astronomical Society. 2021 ; Vol. 501, No. 2. pp. 2969-2982.
Bibtex
@article{015b29b2bdc5402884bc2a6b84f912cf,
title = "Galaxy And Mass Assembly (GAMA): the interplay between galaxy mass, SFR, and heavy element abundance in paired galaxy sets",
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 0 250 km s(-1)) and high multiplicity.",
keywords = "galaxies: abundances, galaxies: star formation, galaxies: interactions, galaxies: statistics, DIGITAL SKY SURVEY, STAR-FORMATION RATE, METALLICITY RELATION, ENVIRONMENT",
author = "Garduno, {L. E.} and Lara-Lopez, {M. A.} and O. Lopez-Cruz and Hopkins, {A. M.} and Owers, {M. S.} and Pimbblet, {K. A.} and Holwerda, {B. W.}",
year = "2021",
month = feb,
day = "1",
doi = "10.1093/mnras/staa3799",
language = "English",
volume = "501",
pages = "2969--2982",
journal = "Royal Astronomical Society. Monthly Notices",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "2",
}
RIS
TY - JOUR
T1 - Galaxy And Mass Assembly (GAMA)
T2 - the interplay between galaxy mass, SFR, and heavy element abundance in paired galaxy sets
AU - Garduno, L. E.
AU - Lara-Lopez, M. A.
AU - Lopez-Cruz, O.
AU - Hopkins, A. M.
AU - Owers, M. S.
AU - Pimbblet, K. A.
AU - Holwerda, B. W.
PY - 2021/2/1
Y1 - 2021/2/1
N2 - 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 0 250 km s(-1)) and high multiplicity.
AB - 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 0 250 km s(-1)) and high multiplicity.
KW - galaxies: abundances
KW - galaxies: star formation
KW - galaxies: interactions
KW - galaxies: statistics
KW - DIGITAL SKY SURVEY
KW - STAR-FORMATION RATE
KW - METALLICITY RELATION
KW - ENVIRONMENT
U2 - 10.1093/mnras/staa3799
DO - 10.1093/mnras/staa3799
M3 - Journal article
VL - 501
SP - 2969
EP - 2982
JO - Royal Astronomical Society. Monthly Notices
JF - Royal Astronomical Society. Monthly Notices
SN - 0035-8711
IS - 2
ER -
