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The properties of inside-out assembled galaxies at z < 0.1

Published online by Cambridge University Press:  29 January 2021

Dejene Zewdie
Affiliation:
Núcleo de Astronomía, Universidad Diego Portales, Santiago, Chile email: dejene.woldeyes@mail.udp.cl Department of Physics, Debre Berhan University (DBU), Debre Berhan, Ethiopia Ethiopian Space Science and Technology Institute-AAU, Addis Ababa, Ethiopia
Mirjana Pović
Affiliation:
Ethiopian Space Science and Technology Institute-AAU, Addis Ababa, Ethiopia Instituto de Astrofisica de Andalucía (IAA-CSIC), Granada, Spain
Manuel Aravena
Affiliation:
Núcleo de Astronomía, Universidad Diego Portales, Santiago, Chile email: dejene.woldeyes@mail.udp.cl
Roberto J. Assef
Affiliation:
Núcleo de Astronomía, Universidad Diego Portales, Santiago, Chile email: dejene.woldeyes@mail.udp.cl
Asrate Gaulle
Affiliation:
Department of Physics, Dilla University, Dilla, Ethiopia
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Abstract

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In this work, we study the properties of galaxies that are showing the inside-out assembly (which we call inside-out assembled galaxies; IOAGs), with the main aim to understand better their properties and morphological transformation. We analysed a sample of galaxies from the Sloan Digital Sky Survey (SDSS) Data Release 8 (DR8), with stellar masses in the range log M* = 10.73 – 11.03 M at at z < 0.1, and analyze their location in the stellar mass-SFR and the color-stellar mass diagram. We found that IOAGs have different spectroscopic properties, most of them being classified either as AGN or composite. We found that the majority of our sources are located below the main sequence of star formation in the SFR-stellar mass diagram, and in the green valley or red sequence in the color-stellar mass diagram. We argue that IOAGs seem to correspond to the transition area where the galaxies are moving from star-forming to quiescent, and from the blue cloud to the red sequence and/or to recently quenched galaxies.

Type
Contributed Papers
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

References

Baldwin, J. A., Phillips, M. M., and Terlevich, R. 1981, PASP, 93, 5 10.1086/130766CrossRefGoogle Scholar
Brinchmann, J., et al., 2004, MNRAS, 351, 1151 CrossRefGoogle Scholar
Kewley, L. J., et al., 2006, MNRAS, 372, 961 10.1111/j.1365-2966.2006.10859.xCrossRefGoogle Scholar
Pérez, E., et al., 2013, ApJ, 764, L1 10.1088/2041-8205/764/1/L1CrossRefGoogle Scholar
Schawinski, K., et al., 2003, MNRAS, 440, 889 10.1093/mnras/stu327CrossRefGoogle Scholar
Whitaker, K. E., et al., 2012, ApJ, 754, L29 10.1088/2041-8205/754/2/L29CrossRefGoogle Scholar
Zewdiw, D., et al. 2020, MNRAS, 498, 4345 10.1093/mnras/staa2488CrossRefGoogle Scholar