THE MAIN SEQUENCES OF STAR-FORMING GALAXIES AND ACTIVE GALACTIC NUCLEI AT HIGH REDSHIFT

被引：40

作者：

Mancuso, C. ^{[1
,2
,3
]}

Lapi, A. ^{[1
,2
,3
]}

Shi, J. ^{[1
,4
]}

Cai, Z. -Y. ^{[4
]}

Gonzalez-Nuevo, J. ^{[5
]}

Bethermin, M. ^{[6
]}

Danese, L. ^{[1
,2
,3
]}

机构：

[1] SISSA, Via Bonomea 265, I-34136 Trieste, Italy

[2] INAF, Osservatorio Astron Trieste, Via Tiepolo 11, I-34131 Trieste, Italy

[3] Ist Nazl Fis Nucl, Sez Trieste, Via Valerio 2, I-34127 Trieste, Italy

[4] Univ Sci & Technol China, Dept Astron, Hefei 230026, Anhui, Peoples R China

[5] Univ Oviedo, Dept Fis, C Calvo Sotelo S-N, E-33007 Oviedo, Spain

[6] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany

来源：

ASTROPHYSICAL JOURNAL | 2016年 / 833卷 / 02期

基金：

美国国家科学基金会;

关键词：

galaxies: evolution; galaxies: formation; quasars: general; BLACK-HOLE MASS; QUASAR LUMINOSITY FUNCTION; DIGITAL-SKY-SURVEY; SIMILAR-TO; SPECTRAL ENERGY-DISTRIBUTIONS; EDDINGTON RATIO DISTRIBUTION; M-ASTERISK RELATION; X-RAY LUMINOSITY; DEEP FIELD-SOUTH; OSCILLATION SPECTROSCOPIC SURVEY;

D O I：

10.3847/1538-4357/833/2/152

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We provide a novel, unifying physical interpretation on the origin, average shape, scatter, and cosmic evolution for the main sequences of star-forming galaxies and active galactic nuclei (AGNs) at high redshift z greater than or similar to 1. We achieve this goal in a model-independent way by exploiting: (i) the redshift-dependent star formation rate functions based on the latest UV/far-IR data from HST/Herschel, and related statistics of strong gravitationally lensed sources; (ii) deterministic evolutionary tracks for the history of star formation and black hole accretion, gauged on a wealth of multiwavelength observations including the observed Eddington ratio distribution. We further validate these ingredients by showing their consistency with the observed galaxy stellar mass functions and AGN bolometric luminosity functions at different redshifts via the continuity equation approach. Our analysis of the main sequence for high-redshift galaxies and AGNs highlights that the present data are consistently interpreted in terms of an in situ coevolution scenario for star formation and black hole accretion, envisaging these as local, time-coordinated processes.

引用

页数：15

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