AGN Feedback Driven Molecular Outflow in NGC 1266

K. Alatalo; K. E. Nyland; G. Graves; S. Deustua; J. Wrobel; L. M. Young; T. A. Davis; M. Bureau; E. Bayet; L. Blitz; M. Bois; F. Bournaud; M. Cappellari; R. L. Davies; P. T. de Zeeuw; E. Emsellem; S. Khochfar; D. Krajnovic; H. Kuntschner; S. Martín; R. M. McDermid; R. Morganti; T. Naab; M. Sarzi; N. Scott; P. Serra; A. Weijmans

doi:10.1017/S1743921312019485

AGN Feedback Driven Molecular Outflow in NGC 1266

K. Alatalo
, K. E. Nyland
, G. Graves
, S. Deustua
, J. Wrobel
, L. M. Young
, T. A. Davis
, M. Bureau
, E. Bayet
, L. Blitz
, M. Bois
, F. Bournaud
, M. Cappellari
, R. L. Davies
, P. T. de Zeeuw
, E. Emsellem
, S. Khochfar
, D. Krajnovic
, H. Kuntschner
, S. Martín

R. M. McDermid, R. Morganti, T. Naab, M. Sarzi, N. Scott, P. Serra, A. Weijmans

Onderzoeksoutput › Academic › peer review

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NGC 1266 is a nearby field galaxy observed as part of the ATLAS3D survey (Cappellari et al. 2011). NGC 1266 has been shown to host a compact (<200 pc) molecular disk and a mass-loaded molecular outflow driven by the AGN (Alatalo et al. 2011). Very Long Basline Array (VLBA) observations at 1.65 GHz revealed a compact (diameter <1.2 pc), high brightness temperature continuum source most consistent with a low-level AGN origin. The VLBA continuum source is positioned at the center of the molecular disk and may be responsible for the expulsion of molecular gas in NGC 1266. Thus, the candidate AGN-driven molecular outflow in NGC 1266 supports the picture in which AGNs do play a significant role in the quenching of star formation and ultimately the evolution of the red sequence of galaxies.

Originele taal-2	English
Titel	Feeding Compact Objects
Subtitel	Accretion on all Scales
Uitgeverij	Cambridge University Press
Pagina's	175-176
Aantal pagina's	2
DOI's	https://doi.org/10.1017/S1743921312019485
Status	Published - feb.-2013
Extern gepubliceerd	Ja

Publicatie series

Naam	IAU Symposium Proceedings Series
Nummer	S290
Volume	8
ISSN van geprinte versie	1743-9213

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10.1017/S1743921312019485

http://adsabs.harvard.edu/abs/2013IAUS..290..175A

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Alatalo, K., Nyland, K. E., Graves, G., Deustua, S., Wrobel, J., Young, L. M., Davis, T. A., Bureau, M., Bayet, E., Blitz, L., Bois, M., Bournaud, F., Cappellari, M., Davies, R. L., de Zeeuw, P. T., Emsellem, E., Khochfar, S., Krajnovic, D., Kuntschner, H., ... Weijmans, A. (2013). AGN Feedback Driven Molecular Outflow in NGC 1266. In Feeding Compact Objects: Accretion on all Scales (blz. 175-176). (IAU Symposium Proceedings Series; Vol. 8, Nr. S290). Cambridge University Press. https://doi.org/10.1017/S1743921312019485

@inproceedings{4b684493acea4a789f8d37fa147ee8e5,

title = "AGN Feedback Driven Molecular Outflow in NGC 1266",

abstract = "NGC 1266 is a nearby field galaxy observed as part of the ATLAS3D survey (Cappellari et al. 2011). NGC 1266 has been shown to host a compact (<200 pc) molecular disk and a mass-loaded molecular outflow driven by the AGN (Alatalo et al. 2011). Very Long Basline Array (VLBA) observations at 1.65 GHz revealed a compact (diameter <1.2 pc), high brightness temperature continuum source most consistent with a low-level AGN origin. The VLBA continuum source is positioned at the center of the molecular disk and may be responsible for the expulsion of molecular gas in NGC 1266. Thus, the candidate AGN-driven molecular outflow in NGC 1266 supports the picture in which AGNs do play a significant role in the quenching of star formation and ultimately the evolution of the red sequence of galaxies.",

keywords = "Galaxies, Active Galactic Nuclei, ISM",

author = "K. Alatalo and Nyland, \{K. E.\} and G. Graves and S. Deustua and J. Wrobel and Young, \{L. M.\} and Davis, \{T. A.\} and M. Bureau and E. Bayet and L. Blitz and M. Bois and F. Bournaud and M. Cappellari and Davies, \{R. L.\} and \{de Zeeuw\}, \{P. T.\} and E. Emsellem and S. Khochfar and D. Krajnovic and H. Kuntschner and S. Mart{\'i}n and McDermid, \{R. M.\} and R. Morganti and T. Naab and M. Sarzi and N. Scott and P. Serra and A. Weijmans",

note = "M1 - Conference Proceedings",

year = "2013",

month = feb,

doi = "10.1017/S1743921312019485",

language = "English",

series = "IAU Symposium Proceedings Series",

publisher = "Cambridge University Press",

number = "S290",

pages = "175--176",

booktitle = "Feeding Compact Objects",

}

Alatalo, K, Nyland, KE, Graves, G, Deustua, S, Wrobel, J, Young, LM, Davis, TA, Bureau, M, Bayet, E, Blitz, L, Bois, M, Bournaud, F, Cappellari, M, Davies, RL, de Zeeuw, PT, Emsellem, E, Khochfar, S, Krajnovic, D, Kuntschner, H, Martín, S, McDermid, RM, Morganti, R, Naab, T, Sarzi, M, Scott, N, Serra, P & Weijmans, A 2013, AGN Feedback Driven Molecular Outflow in NGC 1266. in Feeding Compact Objects: Accretion on all Scales. IAU Symposium Proceedings Series, nr. S290, vol. 8, Cambridge University Press, blz. 175-176. https://doi.org/10.1017/S1743921312019485

TY - GEN

T1 - AGN Feedback Driven Molecular Outflow in NGC 1266

AU - Alatalo, K.

AU - Nyland, K. E.

AU - Graves, G.

AU - Deustua, S.

AU - Wrobel, J.

AU - Young, L. M.

AU - Davis, T. A.

AU - Bureau, M.

AU - Bayet, E.

AU - Blitz, L.

AU - Bois, M.

AU - Bournaud, F.

AU - Cappellari, M.

AU - Davies, R. L.

AU - de Zeeuw, P. T.

AU - Emsellem, E.

AU - Khochfar, S.

AU - Krajnovic, D.

AU - Kuntschner, H.

AU - Martín, S.

AU - McDermid, R. M.

AU - Morganti, R.

AU - Naab, T.

AU - Sarzi, M.

AU - Scott, N.

AU - Serra, P.

AU - Weijmans, A.

N1 - M1 - Conference Proceedings

PY - 2013/2

Y1 - 2013/2

N2 - NGC 1266 is a nearby field galaxy observed as part of the ATLAS3D survey (Cappellari et al. 2011). NGC 1266 has been shown to host a compact (<200 pc) molecular disk and a mass-loaded molecular outflow driven by the AGN (Alatalo et al. 2011). Very Long Basline Array (VLBA) observations at 1.65 GHz revealed a compact (diameter <1.2 pc), high brightness temperature continuum source most consistent with a low-level AGN origin. The VLBA continuum source is positioned at the center of the molecular disk and may be responsible for the expulsion of molecular gas in NGC 1266. Thus, the candidate AGN-driven molecular outflow in NGC 1266 supports the picture in which AGNs do play a significant role in the quenching of star formation and ultimately the evolution of the red sequence of galaxies.

AB - NGC 1266 is a nearby field galaxy observed as part of the ATLAS3D survey (Cappellari et al. 2011). NGC 1266 has been shown to host a compact (<200 pc) molecular disk and a mass-loaded molecular outflow driven by the AGN (Alatalo et al. 2011). Very Long Basline Array (VLBA) observations at 1.65 GHz revealed a compact (diameter <1.2 pc), high brightness temperature continuum source most consistent with a low-level AGN origin. The VLBA continuum source is positioned at the center of the molecular disk and may be responsible for the expulsion of molecular gas in NGC 1266. Thus, the candidate AGN-driven molecular outflow in NGC 1266 supports the picture in which AGNs do play a significant role in the quenching of star formation and ultimately the evolution of the red sequence of galaxies.

KW - Galaxies

KW - Active Galactic Nuclei

KW - ISM

U2 - 10.1017/S1743921312019485

DO - 10.1017/S1743921312019485

M3 - Conference contribution

T3 - IAU Symposium Proceedings Series

SP - 175

EP - 176

BT - Feeding Compact Objects

PB - Cambridge University Press

ER -

AGN Feedback Driven Molecular Outflow in NGC 1266

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