Gas flows in a changing-look AGN

Research output: Contribution to journal › Conference article › Research › peer-review

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Gas flows in a changing-look AGN. / Raimundo, Sandra I.; Bergmann, Thaisa Storchi (Editor); Forman, William (Editor); Overzier, Roderik (Editor); Riffel, Rogério (Editor).

In: Proceedings of the International Astronomical Union, Vol. 15, 2020, p. 334-338.

Research output: Contribution to journal › Conference article › Research › peer-review

Harvard

Raimundo, SI, Bergmann, TS (ed.), Forman, W (ed.), Overzier, R (ed.) & Riffel, R (ed.) 2020, 'Gas flows in a changing-look AGN', Proceedings of the International Astronomical Union, vol. 15, pp. 334-338. https://doi.org/10.1017/S1743921320001672

APA

Raimundo, S. I., Bergmann, T. S. (Ed.), Forman, W. (Ed.), Overzier, R. (Ed.), & Riffel, R. (Ed.) (2020). Gas flows in a changing-look AGN. Proceedings of the International Astronomical Union, 15, 334-338. https://doi.org/10.1017/S1743921320001672

Vancouver

Raimundo SI, Bergmann TS, (ed.), Forman W, (ed.), Overzier R, (ed.), Riffel R, (ed.). Gas flows in a changing-look AGN. Proceedings of the International Astronomical Union. 2020;15:334-338. https://doi.org/10.1017/S1743921320001672

Author

Raimundo, Sandra I. ; Bergmann, Thaisa Storchi (Editor) ; Forman, William (Editor) ; Overzier, Roderik (Editor) ; Riffel, Rogério (Editor). / Gas flows in a changing-look AGN. In: Proceedings of the International Astronomical Union. 2020 ; Vol. 15. pp. 334-338.

Bibtex

@inproceedings{97cf975a30a64a908b15fbed01cbcb16,
title = "Gas flows in a changing-look AGN",
abstract = "The galaxy Mrk 590 is one of the few known 'changing-look' Active Galactic Nuclei (AGN) to have transitioned between states twice, having just increased its flux after a period of ∼ 10 years of low activity. In addition to the increase in flux, the optical broad emission lines have reappeared but show a different profile than what was observed before they disappeared. The gas motions in the host galaxy of this changing-look AGN show outflows and dynamical structures able to drive gas to the nucleus, suggesting an interplay between inflow and outflow in the centre of the galaxy.",
keywords = "galaxies:active, galaxies:individual(Mrk 590), galaxies:nuclei",
author = "Raimundo, {Sandra I.} and Bergmann, {Thaisa Storchi} and William Forman and Roderik Overzier and Rog{\'e}rio Riffel",
note = "Publisher Copyright: {\textcopyright} The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union.",
year = "2020",
doi = "10.1017/S1743921320001672",
language = "English",
volume = "15",
pages = "334--338",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",

}

RIS

TY - GEN

T1 - Gas flows in a changing-look AGN

AU - Raimundo, Sandra I.

A2 - Bergmann, Thaisa Storchi

A2 - Forman, William

A2 - Overzier, Roderik

A2 - Riffel, Rogério

N1 - Publisher Copyright: © The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union.

PY - 2020

Y1 - 2020

N2 - The galaxy Mrk 590 is one of the few known 'changing-look' Active Galactic Nuclei (AGN) to have transitioned between states twice, having just increased its flux after a period of ∼ 10 years of low activity. In addition to the increase in flux, the optical broad emission lines have reappeared but show a different profile than what was observed before they disappeared. The gas motions in the host galaxy of this changing-look AGN show outflows and dynamical structures able to drive gas to the nucleus, suggesting an interplay between inflow and outflow in the centre of the galaxy.

AB - The galaxy Mrk 590 is one of the few known 'changing-look' Active Galactic Nuclei (AGN) to have transitioned between states twice, having just increased its flux after a period of ∼ 10 years of low activity. In addition to the increase in flux, the optical broad emission lines have reappeared but show a different profile than what was observed before they disappeared. The gas motions in the host galaxy of this changing-look AGN show outflows and dynamical structures able to drive gas to the nucleus, suggesting an interplay between inflow and outflow in the centre of the galaxy.

KW - galaxies:active

KW - galaxies:individual(Mrk 590)

KW - galaxies:nuclei

U2 - 10.1017/S1743921320001672

DO - 10.1017/S1743921320001672

M3 - Conference article

AN - SCOPUS:85103462516

VL - 15

SP - 334

EP - 338

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

ER -

ID: 271830236