Structure and kinematics of early-type galaxies from integral field spectroscopy

M Cappellari - Annual review of astronomy and astrophysics, 2016 - annualreviews.org
Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …

Stellar population diagnostics of elliptical galaxy formation

A Renzini - Annu. Rev. Astron. Astrophys., 2006 - annualreviews.org
Major progress has been achieved in recent years in mapping the properties of passively-
evolving, early-type galaxies (ETG) from the local universe all the way to redshift∼ 2. Here …

The ATLAS3D project – XV. Benchmark for early-type galaxies scaling relations from 260 dynamical models: mass-to-light ratio, dark matter, Fundamental Plane and …

M Cappellari, N Scott, K Alatalo, L Blitz… - Monthly Notices of …, 2013 - academic.oup.com
We study the volume-limited and nearly mass-selected (stellar mass M stars≳ 6× 109 M⊙)
ATLAS3D sample of 260 early-type galaxies (ETGs, ellipticals Es and lenticulars S0s). We …

[图书][B] Galaxy formation and evolution

H Mo, F Van den Bosch, S White - 2010 - books.google.com
The rapidly expanding field of galaxy formation lies at the interface between astronomy,
particle physics, and cosmology. Covering diverse topics from these disciplines, all of which …

On the maximum luminosity of galaxies and their central black holes: feedback from momentum-driven winds

N Murray, E Quataert, TA Thompson - The Astrophysical Journal, 2005 - iopscience.iop.org
We investigate large-scale galactic winds driven by momentum deposition. Momentum
injection is provided by (1) radiation pressure produced by the continuum absorption and …

The SAURON project—IV. The mass-to-light ratio, the virial mass estimator and the Fundamental Plane of elliptical and lenticular galaxies

M Cappellari, R Bacon, M Bureau… - Monthly Notices of …, 2006 - academic.oup.com
We investigate the well-known correlations between the dynamical mass-to-light ratio (M/L)
and other global observables of elliptical (E) and lenticular (S0) galaxies. We construct two …

Dynamical family properties and dark halo scaling relations of giant elliptical galaxies

O Gerhard, A Kronawitter, RP Saglia… - The Astronomical …, 2001 - iopscience.iop.org
Based on a uniform dynamical analysis of the line-profile shapes of 21 mostly luminous,
slowly rotating, and nearly round elliptical galaxies, we have investigated the dynamical …

How special are brightest group and cluster galaxies?

A Von Der Linden, PN Best… - Monthly Notices of …, 2007 - academic.oup.com
Abstract We use the Sloan Digital Sky Survey (SDSS) to construct a sample of 625 brightest
group and cluster galaxies (BCGs) together with control samples of non-BCGs matched in …

Early-type galaxies in the sloan digital sky survey. iii. the fundamental plane

M Bernardi, RK Sheth, J Annis, S Burles… - The Astronomical …, 2003 - iopscience.iop.org
A magnitude-limited sample of nearly 9000 early-type galaxies in the redshift range 0.01≤
z≤ 0.3 was selected from the Sloan Digital Sky Survey (SDSS) using morphological and …

An over-massive black hole in the compact lenticular galaxy NGC 1277

RCE van den Bosch, K Gebhardt, K Gültekin… - Nature, 2012 - nature.com
Most massive galaxies have supermassive black holes at their centres, and the masses of
the black holes are believed to correlate with properties of the host-galaxy bulge component …