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. DaviesP. 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

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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 (~ 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",

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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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