Gas reservoir of a hyper-luminous quasar at z = 2.6

C. Feruglio, A. Bongiorno, F. Fiore, M. Krips, M. Brusa, E. Daddi, I. Gavignaud, R. Maiolino, E. Piconcelli, M. Sargent, C. Vignali, L. Zappacosta

Resultado de la investigación: Article

14 Citas (Scopus)

Resumen

Context. Understanding the relationship between the formation and evolution of galaxies and their central super-massive black holes (SMBH) is one of the main topics in extragalactic astrophysics. Links and feedback may reciprocally affect both black hole and galaxy growth. Aims. Observations of the CO line at the main epoch of galaxy and SMBH assembly (z = 2-4) are crucial to investigating the gas mass, star formation, and accretion onto SMBHs, and the effect of AGN feedback. Potential correlations between AGN and host galaxy properties can be highlighted by observing extreme objects. Methods. We targeted CO(3-2) in ULAS J1539+0557, a hyper-luminous quasar (Lbol > 1048 erg/s) at z = 2.658, selected through its unusual red colour in the UKIDSS Large Area Survey (ULAS). Results. We find a molecular gas mass of 4.1 ± 0.8 × 1010 M, by adopting a conversion factor α = 0.8 M K-1 km s -1 pc2, and a gas fraction of ~0.4-0.1, depending mostly on the assumed source inclination. We also find a robust lower limit to the star-formation rate (SFR = 250-1600 M/yr) and star-formation efficiency (SFE = 25-350 L/(K kms-1pc2) by comparing the observed optical-near-infrared spectral energy distribution with AGN and galaxy templates. The black hole gas consumption timescale, M(H2)/acc, is ~160 Myr, similar to or higher than the gas consumption timescale. Conclusions. The gas content and the star formation efficiency are similar to those of other high-luminosity, highly obscured quasars, and at the lower end of the star-formation efficiency of unobscured quasars, in line with predictions from AGN-galaxy co-evolutionary scenarios. Further measurements of the (sub)mm continuum in this and similar sources are mandatory to obtain a robust observational picture of the AGN evolutionary sequence.

Idioma originalEnglish
Número de artículoA91
PublicaciónAstronomy and Astrophysics
Volumen565
DOI
EstadoPublished - 2014

Huella dactilar

quasars
galaxies
star formation
gases
gas
timescale
astrophysics
molecular gases
star formation rate
spectral energy distribution
erg
inclination
gas reservoir
near infrared
templates
assembly
accretion
luminosity
time measurement
continuums

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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Feruglio, C., Bongiorno, A., Fiore, F., Krips, M., Brusa, M., Daddi, E., ... Zappacosta, L. (2014). Gas reservoir of a hyper-luminous quasar at z = 2.6. Astronomy and Astrophysics, 565, [A91]. https://doi.org/10.1051/0004-6361/201423719
Feruglio, C. ; Bongiorno, A. ; Fiore, F. ; Krips, M. ; Brusa, M. ; Daddi, E. ; Gavignaud, I. ; Maiolino, R. ; Piconcelli, E. ; Sargent, M. ; Vignali, C. ; Zappacosta, L. / Gas reservoir of a hyper-luminous quasar at z = 2.6. En: Astronomy and Astrophysics. 2014 ; Vol. 565.
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abstract = "Context. Understanding the relationship between the formation and evolution of galaxies and their central super-massive black holes (SMBH) is one of the main topics in extragalactic astrophysics. Links and feedback may reciprocally affect both black hole and galaxy growth. Aims. Observations of the CO line at the main epoch of galaxy and SMBH assembly (z = 2-4) are crucial to investigating the gas mass, star formation, and accretion onto SMBHs, and the effect of AGN feedback. Potential correlations between AGN and host galaxy properties can be highlighted by observing extreme objects. Methods. We targeted CO(3-2) in ULAS J1539+0557, a hyper-luminous quasar (Lbol > 1048 erg/s) at z = 2.658, selected through its unusual red colour in the UKIDSS Large Area Survey (ULAS). Results. We find a molecular gas mass of 4.1 ± 0.8 × 1010 M⊙, by adopting a conversion factor α = 0.8 M⊙ K-1 km s -1 pc2, and a gas fraction of ~0.4-0.1, depending mostly on the assumed source inclination. We also find a robust lower limit to the star-formation rate (SFR = 250-1600 M⊙/yr) and star-formation efficiency (SFE = 25-350 L⊙/(K kms-1pc2) by comparing the observed optical-near-infrared spectral energy distribution with AGN and galaxy templates. The black hole gas consumption timescale, M(H2)/acc, is ~160 Myr, similar to or higher than the gas consumption timescale. Conclusions. The gas content and the star formation efficiency are similar to those of other high-luminosity, highly obscured quasars, and at the lower end of the star-formation efficiency of unobscured quasars, in line with predictions from AGN-galaxy co-evolutionary scenarios. Further measurements of the (sub)mm continuum in this and similar sources are mandatory to obtain a robust observational picture of the AGN evolutionary sequence.",
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Feruglio, C, Bongiorno, A, Fiore, F, Krips, M, Brusa, M, Daddi, E, Gavignaud, I, Maiolino, R, Piconcelli, E, Sargent, M, Vignali, C & Zappacosta, L 2014, 'Gas reservoir of a hyper-luminous quasar at z = 2.6', Astronomy and Astrophysics, vol. 565, A91. https://doi.org/10.1051/0004-6361/201423719

Gas reservoir of a hyper-luminous quasar at z = 2.6. / Feruglio, C.; Bongiorno, A.; Fiore, F.; Krips, M.; Brusa, M.; Daddi, E.; Gavignaud, I.; Maiolino, R.; Piconcelli, E.; Sargent, M.; Vignali, C.; Zappacosta, L.

En: Astronomy and Astrophysics, Vol. 565, A91, 2014.

Resultado de la investigación: Article

TY - JOUR

T1 - Gas reservoir of a hyper-luminous quasar at z = 2.6

AU - Feruglio, C.

AU - Bongiorno, A.

AU - Fiore, F.

AU - Krips, M.

AU - Brusa, M.

AU - Daddi, E.

AU - Gavignaud, I.

AU - Maiolino, R.

AU - Piconcelli, E.

AU - Sargent, M.

AU - Vignali, C.

AU - Zappacosta, L.

PY - 2014

Y1 - 2014

N2 - Context. Understanding the relationship between the formation and evolution of galaxies and their central super-massive black holes (SMBH) is one of the main topics in extragalactic astrophysics. Links and feedback may reciprocally affect both black hole and galaxy growth. Aims. Observations of the CO line at the main epoch of galaxy and SMBH assembly (z = 2-4) are crucial to investigating the gas mass, star formation, and accretion onto SMBHs, and the effect of AGN feedback. Potential correlations between AGN and host galaxy properties can be highlighted by observing extreme objects. Methods. We targeted CO(3-2) in ULAS J1539+0557, a hyper-luminous quasar (Lbol > 1048 erg/s) at z = 2.658, selected through its unusual red colour in the UKIDSS Large Area Survey (ULAS). Results. We find a molecular gas mass of 4.1 ± 0.8 × 1010 M⊙, by adopting a conversion factor α = 0.8 M⊙ K-1 km s -1 pc2, and a gas fraction of ~0.4-0.1, depending mostly on the assumed source inclination. We also find a robust lower limit to the star-formation rate (SFR = 250-1600 M⊙/yr) and star-formation efficiency (SFE = 25-350 L⊙/(K kms-1pc2) by comparing the observed optical-near-infrared spectral energy distribution with AGN and galaxy templates. The black hole gas consumption timescale, M(H2)/acc, is ~160 Myr, similar to or higher than the gas consumption timescale. Conclusions. The gas content and the star formation efficiency are similar to those of other high-luminosity, highly obscured quasars, and at the lower end of the star-formation efficiency of unobscured quasars, in line with predictions from AGN-galaxy co-evolutionary scenarios. Further measurements of the (sub)mm continuum in this and similar sources are mandatory to obtain a robust observational picture of the AGN evolutionary sequence.

AB - Context. Understanding the relationship between the formation and evolution of galaxies and their central super-massive black holes (SMBH) is one of the main topics in extragalactic astrophysics. Links and feedback may reciprocally affect both black hole and galaxy growth. Aims. Observations of the CO line at the main epoch of galaxy and SMBH assembly (z = 2-4) are crucial to investigating the gas mass, star formation, and accretion onto SMBHs, and the effect of AGN feedback. Potential correlations between AGN and host galaxy properties can be highlighted by observing extreme objects. Methods. We targeted CO(3-2) in ULAS J1539+0557, a hyper-luminous quasar (Lbol > 1048 erg/s) at z = 2.658, selected through its unusual red colour in the UKIDSS Large Area Survey (ULAS). Results. We find a molecular gas mass of 4.1 ± 0.8 × 1010 M⊙, by adopting a conversion factor α = 0.8 M⊙ K-1 km s -1 pc2, and a gas fraction of ~0.4-0.1, depending mostly on the assumed source inclination. We also find a robust lower limit to the star-formation rate (SFR = 250-1600 M⊙/yr) and star-formation efficiency (SFE = 25-350 L⊙/(K kms-1pc2) by comparing the observed optical-near-infrared spectral energy distribution with AGN and galaxy templates. The black hole gas consumption timescale, M(H2)/acc, is ~160 Myr, similar to or higher than the gas consumption timescale. Conclusions. The gas content and the star formation efficiency are similar to those of other high-luminosity, highly obscured quasars, and at the lower end of the star-formation efficiency of unobscured quasars, in line with predictions from AGN-galaxy co-evolutionary scenarios. Further measurements of the (sub)mm continuum in this and similar sources are mandatory to obtain a robust observational picture of the AGN evolutionary sequence.

KW - Galaxies: active

KW - Galaxies: evolution

KW - Quasars: emission lines

KW - Quasars: general

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DO - 10.1051/0004-6361/201423719

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Feruglio C, Bongiorno A, Fiore F, Krips M, Brusa M, Daddi E y otros. Gas reservoir of a hyper-luminous quasar at z = 2.6. Astronomy and Astrophysics. 2014;565. A91. https://doi.org/10.1051/0004-6361/201423719