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Observational evidence for AGN feedback in early-type galaxies

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The definitive version of the book is available at www.blackwell-synergy.com. Copyright Blackwell Publishing as discussed by the authors, 2017. All rights reserved. And the book can be found here.
Abstract
The definitive version is available at www.blackwell-synergy.com. Copyright Blackwell Publishing

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Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies

TL;DR: In this paper, supermassive black holes (BHs) have been found in 85 galaxies by dynamical modeling of spatially resolved kinematics, and it has been shown that BHs and bulges coevolve by regulating each other's growth.
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Observational Evidence of Active Galactic Nuclei Feedback

TL;DR: In this article, it was shown that the radiative or quasar mode of feedback can account for the observed proportionality between the central black hole and the host galaxy mass, which can lead to ejection or heating of the gas.
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Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies: Supplemental Material

TL;DR: Kormendy and Ho as mentioned in this paper proposed a method to estimate the BH masses for galaxies with active nuclei (AGNs) based on the observational criteria that are used to classify classical and pseudo bulges.
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Galaxy Zoo: morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey

TL;DR: Galaxy Zoo as mentioned in this paper provides visual morphological classifications for nearly one million galaxies, extracted from the Sloan Digital Sky Survey (SDSS), which was made possible by inviting the general public to visually inspect and classify these galaxies via the internet.

Dwarf galaxies, cold dark matter, and biased galaxy formation

Avishai Dekel, +1 more
TL;DR: In this article, a reexamination is conducted of the formation of dwarf, diffuse, metal-poor galaxies due to supernova-driven winds, in view of data on the systematic properties of dwarfs in the Local Group and Virgo Cluster.
References
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The Sloan Digital Sky Survey: Technical Summary

Donald G. York
- 27 Jun 2000 - 
TL;DR: The Sloan Digital Sky Survey (SDSS) as mentioned in this paper provides the data to support detailed investigations of the distribution of luminous and non-luminous matter in the Universe: a photometrically and astrometrically calibrated digital imaging survey of pi steradians above about Galactic latitude 30 degrees in five broad optical bands.
Journal ArticleDOI

The Sloan Digital Sky Survey: Technical summary

Donald G. York, +151 more
TL;DR: The Sloan Digital Sky Survey (SDSS) as discussed by the authors provides the data to support detailed investigations of the distribution of luminous and non-luminous matter in the universe: a photometrically and astrometrically calibrated digital imaging survey of π sr above about Galactic latitude 30° in five broad optical bands to a depth of g' ~ 23 mag.
Journal ArticleDOI

The Global Schmidt law in star forming galaxies

TL;DR: In this paper, the Schmidt law was used to model the global star formation law over the full range of gas densities and star formation rates observed in galaxies, and the results showed that the SFR scales with the ratio of the gas density to the average orbital timescale.
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The Dust Content and Opacity of Actively Star-Forming Galaxies

TL;DR: In this article, far-infrared (FIR) photometry at 150 and 205 micron(s) of eight low-redshift starburst galaxies obtained with the Infrared Space Observatory (ISO) ISOPHOT is presented.
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The Sloan Digital Sky Survey: Technical summary

Donald G. York, +151 more