The evolution of the oxygen radial gradients in spiral galaxies

M. Mollá; O. Cavichia; B. Gibson; P. Tissera; P. Sánchez-Blázquez; A. I. Díaz; Y. Ascasibar; C. G. Few; S. F. Sánchez; W. J. MacIel

doi:10.1017/S1743921319004290

The evolution of the oxygen radial gradients in spiral galaxies

M. Mollá, O. Cavichia, B. Gibson, P. Tissera, P. Sánchez-Blázquez, A. I. Díaz, Y. Ascasibar, C. G. Few, S. F. Sánchez, W. J. MacIel

Research output: Contribution to journal › Article › peer-review

Abstract

We analyse the evolution with redshift of the radial gradient of oxygen abundances in spiral disks resulting from our MULCHEM chemical evolution models, computed for galaxies of different sizes or masses, studying the relationships between the gradients and galaxy characteristics as the stellar mass, the size, the gas fraction or the star formation rate for z < 4.

Original language	English
Number of pages	1
Journal	Proceedings of the International Astronomical Union
Volume	14
Issue number	A30
DOIs	https://doi.org/10.1017/S1743921319004290
Publication status	Published - 1 Jan 2018
Externally published	Yes

Keywords

Galaxies: Abundances
Galaxies: Formation
Galaxies: Spirals

ASJC Scopus subject areas

Medicine (miscellaneous)
Astronomy and Astrophysics
Nutrition and Dietetics
Public Health, Environmental and Occupational Health
Space and Planetary Science

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

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10.1017/S1743921319004290

Cite this

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title = "The evolution of the oxygen radial gradients in spiral galaxies",

abstract = "We analyse the evolution with redshift of the radial gradient of oxygen abundances in spiral disks resulting from our MULCHEM chemical evolution models, computed for galaxies of different sizes or masses, studying the relationships between the gradients and galaxy characteristics as the stellar mass, the size, the gas fraction or the star formation rate for z < 4.",

keywords = "Galaxies: Abundances, Galaxies: Formation, Galaxies: Spirals",

author = "M. Moll{\'a} and O. Cavichia and B. Gibson and P. Tissera and P. S{\'a}nchez-Bl{\'a}zquez and D{\'i}az, {A. I.} and Y. Ascasibar and Few, {C. G.} and S{\'a}nchez, {S. F.} and MacIel, {W. J.}",

year = "2018",

month = jan,

day = "1",

doi = "10.1017/S1743921319004290",

language = "English",

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journal = "Proceedings of the International Astronomical Union",

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TY - JOUR

T1 - The evolution of the oxygen radial gradients in spiral galaxies

AU - Mollá, M.

AU - Cavichia, O.

AU - Gibson, B.

AU - Tissera, P.

AU - Sánchez-Blázquez, P.

AU - Díaz, A. I.

AU - Ascasibar, Y.

AU - Few, C. G.

AU - Sánchez, S. F.

AU - MacIel, W. J.

PY - 2018/1/1

Y1 - 2018/1/1

N2 - We analyse the evolution with redshift of the radial gradient of oxygen abundances in spiral disks resulting from our MULCHEM chemical evolution models, computed for galaxies of different sizes or masses, studying the relationships between the gradients and galaxy characteristics as the stellar mass, the size, the gas fraction or the star formation rate for z < 4.

AB - We analyse the evolution with redshift of the radial gradient of oxygen abundances in spiral disks resulting from our MULCHEM chemical evolution models, computed for galaxies of different sizes or masses, studying the relationships between the gradients and galaxy characteristics as the stellar mass, the size, the gas fraction or the star formation rate for z < 4.

KW - Galaxies: Abundances

KW - Galaxies: Formation

KW - Galaxies: Spirals

UR - http://www.scopus.com/inward/record.url?scp=85080882061&partnerID=8YFLogxK

U2 - 10.1017/S1743921319004290

DO - 10.1017/S1743921319004290

M3 - Article

AN - SCOPUS:85080882061

VL - 14

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - A30

ER -

The evolution of the oxygen radial gradients in spiral galaxies

Abstract

Keywords

ASJC Scopus subject areas

UN SDGs

Access to Document

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