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Selection and characterisation of Red Geysers in the MaNGA survey

Published online by Cambridge University Press:  29 March 2021

Gabriele S. Ilha Open the ORCID record for Gabriele S. Ilha [Opens in a new window] ,
Rogemar Riffel ,
Sandro B. Rembold  and
Jáderson S. Schimóia
Gabriele S. Ilha
Affiliation:
Universidade Federal de Santa Maria, Departamento de Física, Centro de Ciências Naturais e Exatas, 97105-900, Santa Maria, RS, Brazil email: [email protected] Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
Rogemar Riffel
Affiliation:
Universidade Federal de Santa Maria, Departamento de Física, Centro de Ciências Naturais e Exatas, 97105-900, Santa Maria, RS, Brazil email: [email protected] Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
Sandro B. Rembold
Affiliation:
Universidade Federal de Santa Maria, Departamento de Física, Centro de Ciências Naturais e Exatas, 97105-900, Santa Maria, RS, Brazil email: [email protected] Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
Jáderson S. Schimóia
Affiliation:
Universidade Federal de Santa Maria, Departamento de Física, Centro de Ciências Naturais e Exatas, 97105-900, Santa Maria, RS, Brazil email: [email protected] Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
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Abstract

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Red Geysers are quiescent galaxies that show a bi-polar outflow, but the mechanism that produces this outflow is still unclear. Using MaNGA data, we find that Red Geysers correspond to ∼1.6% of the sample of galaxies already observed by MaNGA. About ∼16% of the Red Geysers show clear evidence of Active Galactic Nuclei, as revealed by emission-line ratios.

Keywords

galaxies: red geysersgalaxies: kinematicsgalaxies: nuclei
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 433 - 435
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

References

Abolfathi, B., et al. 2018, ApJS, 235, 42 CrossRefGoogle Scholar
Aguado, , et al. 2019, ApJS, 240, 23 CrossRefGoogle Scholar
Baldwin, J. A., Phillips, M. M., Terlevich, R., et al. 1981, PASP, 93, 5CrossRefGoogle Scholar
Cheung, E., et al. 2016, Nature, 533, 504 CrossRefGoogle Scholar
Cid Fernandes, R., et al. 2010, MNRAS, 403, 1036 CrossRefGoogle Scholar
Krajnović, , et al. 2006, MNRAS, 366, 787 CrossRefGoogle Scholar
Riffel, R. A., et al. 2019, MNRAS, 485, 5590 CrossRefGoogle Scholar
Roy, N., et al. 2018, ApJ, 869, 117 CrossRefGoogle Scholar