NGC 1266 as a local candidate for rapid cessation of star formation

Katherine Alatalo; Kristina Nyland; Genevieve Graves; Susana Deustua; Kristen Shapiro Griffin; Pierre-Alain Duc; Michele Cappellari; Richard M. McDermid; Timothy A. Davis; Alison F. Crocker; Lisa M. Young; Philip Chang; Nicholas Scott; Sabrina L. Cales; Estelle Bayet; Leo Blitz; Maxime Bois; Frédéric Bournaud; Martin Bureau; Roger L. Davies; P. T. de Zeeuw; Eric Emsellem; Sadegh Khochfar; Davor Krajnović; Harald Kuntschner; Raffaella Morganti; Thorsten Naab; Tom Oosterloo; Marc Sarzi; Paolo Serra; Anne-Marie Weijmans

doi:10.1088/0004-637X/780/2/186

NGC 1266 as a local candidate for rapid cessation of star formation

Katherine Alatalo
, Kristina Nyland
, Genevieve Graves
, Susana Deustua
, Kristen Shapiro Griffin
, Pierre-Alain Duc
, Michele Cappellari
, Richard M. McDermid
, Timothy A. Davis
, Alison F. Crocker
, Lisa M. Young
, Philip Chang
, Nicholas Scott
, Sabrina L. Cales
, Estelle Bayet
, Leo Blitz
, Maxime Bois
, Frédéric Bournaud
, Martin Bureau
, Roger L. Davies

P. T. de Zeeuw, Eric Emsellem, Sadegh Khochfar, Davor Krajnović, Harald Kuntschner, Raffaella Morganti, Thorsten Naab, Tom Oosterloo, Marc Sarzi, Paolo Serra, Anne-Marie Weijmans

School of Physics and Astronomy

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

Abstract

We present new Spectrographic Areal Unit for Research on Optical Nebulae (SAURON) integral-field spectroscopy and Swift Ultraviolet Optical Telescope (UVOT) observations of molecular outflow host galaxy NGC 1266 that indicate NGC 1266 has experienced a rapid cessation of star formation. Both the SAURON maps of stellar population age and the Swift UVOT observations demonstrate the presence of young (~ 1 Gyr by cyclically injecting turbulent energy into the dense molecular gas via a radio jet, inhibiting star formation.

Original language	English
Article number	186
Number of pages	10
Journal	Astrophysical Journal
Volume	780
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/780/2/186
Publication status	Published - 23 Dec 2013

Keywords

Galaxies: active
Galaxies: evolution
Galaxies: individual: NGC 1266

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10.1088/0004-637X/780/2/186

astroph_1311.6469
© 2013. The American Astronomical Society. All rights reserved. This is an Accepted Manuscript of an article published online in the Astrophysical Journal on 23 December 2013, available online: http://iopscience.iop.org/0004-637X/780/2/186/
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Alatalo, K., Nyland, K., Graves, G., Deustua, S., Shapiro Griffin, K., Duc, P.-A., Cappellari, M., McDermid, R. M., Davis, T. A., Crocker, A. F., Young, L. M., Chang, P., Scott, N., Cales, S. L., Bayet, E., Blitz, L., Bois, M., Bournaud, F., Bureau, M., ... Weijmans, A.-M. (2013). NGC 1266 as a local candidate for rapid cessation of star formation. Astrophysical Journal, 780(2), Article 186. https://doi.org/10.1088/0004-637X/780/2/186

@article{f04086752ece4919906dd14c1ee2e5ef,

title = "NGC 1266 as a local candidate for rapid cessation of star formation",

abstract = "We present new Spectrographic Areal Unit for Research on Optical Nebulae (SAURON) integral-field spectroscopy and Swift Ultraviolet Optical Telescope (UVOT) observations of molecular outflow host galaxy NGC 1266 that indicate NGC 1266 has experienced a rapid cessation of star formation. Both the SAURON maps of stellar population age and the Swift UVOT observations demonstrate the presence of young (\textasciitilde{} 1 Gyr by cyclically injecting turbulent energy into the dense molecular gas via a radio jet, inhibiting star formation.",

keywords = "Galaxies: active, Galaxies: evolution, Galaxies: individual: NGC 1266",

author = "Katherine Alatalo and Kristina Nyland and Genevieve Graves and Susana Deustua and \{Shapiro Griffin\}, Kristen and Pierre-Alain Duc and Michele Cappellari and McDermid, \{Richard M.\} and Davis, \{Timothy A.\} and Crocker, \{Alison F.\} and Young, \{Lisa M.\} and Philip Chang and Nicholas Scott and Cales, \{Sabrina L.\} and Estelle Bayet and Leo Blitz and Maxime Bois and Fr{\'e}d{\'e}ric Bournaud and Martin Bureau and Davies, \{Roger L.\} and \{de Zeeuw\}, \{P. T.\} and Eric Emsellem and Sadegh Khochfar and Davor Krajnovi{\'c} and Harald Kuntschner and Raffaella Morganti and Thorsten Naab and Tom Oosterloo and Marc Sarzi and Paolo Serra and Anne-Marie Weijmans",

year = "2013",

month = dec,

day = "23",

doi = "10.1088/0004-637X/780/2/186",

language = "English",

volume = "780",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "2",

}

Alatalo, K, Nyland, K, Graves, G, Deustua, S, Shapiro Griffin, K, Duc, P-A, Cappellari, M, McDermid, RM, Davis, TA, Crocker, AF, Young, LM, Chang, P, Scott, N, Cales, SL, Bayet, E, Blitz, L, Bois, M, Bournaud, F, Bureau, M, Davies, RL, de Zeeuw, PT, Emsellem, E, Khochfar, S, Krajnović, D, Kuntschner, H, Morganti, R, Naab, T, Oosterloo, T, Sarzi, M, Serra, P & Weijmans, A-M 2013, 'NGC 1266 as a local candidate for rapid cessation of star formation', Astrophysical Journal, vol. 780, no. 2, 186. https://doi.org/10.1088/0004-637X/780/2/186

TY - JOUR

T1 - NGC 1266 as a local candidate for rapid cessation of star formation

AU - Alatalo, Katherine

AU - Nyland, Kristina

AU - Graves, Genevieve

AU - Deustua, Susana

AU - Shapiro Griffin, Kristen

AU - Duc, Pierre-Alain

AU - Cappellari, Michele

AU - McDermid, Richard M.

AU - Davis, Timothy A.

AU - Crocker, Alison F.

AU - Young, Lisa M.

AU - Chang, Philip

AU - Scott, Nicholas

AU - Cales, Sabrina L.

AU - Bayet, Estelle

AU - Blitz, Leo

AU - Bois, Maxime

AU - Bournaud, Frédéric

AU - Bureau, Martin

AU - Davies, Roger L.

AU - de Zeeuw, P. T.

AU - Emsellem, Eric

AU - Khochfar, Sadegh

AU - Krajnović, Davor

AU - Kuntschner, Harald

AU - Morganti, Raffaella

AU - Naab, Thorsten

AU - Oosterloo, Tom

AU - Sarzi, Marc

AU - Serra, Paolo

AU - Weijmans, Anne-Marie

PY - 2013/12/23

Y1 - 2013/12/23

N2 - We present new Spectrographic Areal Unit for Research on Optical Nebulae (SAURON) integral-field spectroscopy and Swift Ultraviolet Optical Telescope (UVOT) observations of molecular outflow host galaxy NGC 1266 that indicate NGC 1266 has experienced a rapid cessation of star formation. Both the SAURON maps of stellar population age and the Swift UVOT observations demonstrate the presence of young (~ 1 Gyr by cyclically injecting turbulent energy into the dense molecular gas via a radio jet, inhibiting star formation.

AB - We present new Spectrographic Areal Unit for Research on Optical Nebulae (SAURON) integral-field spectroscopy and Swift Ultraviolet Optical Telescope (UVOT) observations of molecular outflow host galaxy NGC 1266 that indicate NGC 1266 has experienced a rapid cessation of star formation. Both the SAURON maps of stellar population age and the Swift UVOT observations demonstrate the presence of young (~ 1 Gyr by cyclically injecting turbulent energy into the dense molecular gas via a radio jet, inhibiting star formation.

KW - Galaxies: active

KW - Galaxies: evolution

KW - Galaxies: individual: NGC 1266

UR - http://adsabs.harvard.edu/abs/2014ApJ...780..186A

U2 - 10.1088/0004-637X/780/2/186

DO - 10.1088/0004-637X/780/2/186

M3 - Article

SN - 0004-637X

VL - 780

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 186

ER -

NGC 1266 as a local candidate for rapid cessation of star formation

Abstract

Keywords

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