scholarly journals Structure and Kinematics of Early-Type Galaxies from Integral Field Spectroscopy

2016 ◽  
Vol 54 (1) ◽  
pp. 597-665 ◽  
Author(s):  
Michele Cappellari
Keyword(s):  
Early Type ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field

scholarly journals The stellar structure of early-type galaxies: a wide-field Mitchell Spectrograph view

2016 ◽  
Vol 11 (S321) ◽  
pp. 288-288
Author(s):  
N. F. Boardman ◽  
A. Weijmans ◽  
R. C. E. van den Bosch ◽  
L. Zhu ◽  
A. Yildirim ◽  
...  
Keyword(s):  
Effective Radius ◽  
Stellar Structure ◽  
Wide Field ◽  
Early Type ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field ◽  
Made In

Much progress has been made in recent years towards understanding how early-type galaxies (ETGs) form and evolve. SAURON (Bacon et al. 2001) integral-field spectroscopy from the ATLAS3D survey (Cappellari et al. 2011) has suggested that less massive ETGs are linked directly to spirals, whereas the most massive objects appear to form from a series of merging and accretion events (Cappellari et al. 2013). However, the ATLAS3D data typically only extends to about one half-light radius (or effective radius, Re), making it unclear if this picture is truly complete.

scholarly journals Integral-Field Spectroscopic Surveys of Nearby Early–type Galaxies

2010 ◽  
Vol 6 (S277) ◽  
pp. 83-88
Author(s):  
Eric Emsellem
Keyword(s):  
Early Type ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field

AbstractI briefly review here a few past or on-going surveys of nearby ETGs via integral-field spectroscopy, focusing on their dynamical status, evolution, and stellar/gaseous content.

scholarly journals VIMOS mosaic integral-field spectroscopy of the bulge and disc of the early-type galaxy NGC 4697

2015 ◽  
Vol 452 (1) ◽  
pp. 99-114 ◽  
Author(s):  
C. Spiniello ◽  
N. R. Napolitano ◽  
L. Coccato ◽  
V. Pota ◽  
A. J. Romanowsky ◽  
...  
Keyword(s):  
Early Type ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field ◽  
Early Type Galaxy

scholarly journals Spiral galaxies in the SAURON survey

2007 ◽  
Vol 3 (S245) ◽  
pp. 271-276
Author(s):  
Reynier F. Peletier ◽  
Katia Ganda ◽  
Jesús Falcón-Barroso ◽  
Roland Bacon ◽  
Michele Cappellari ◽  
...  
Keyword(s):  
Radial Velocity ◽  
Velocity Dispersion ◽  
Spiral Galaxies ◽  
Line Strength ◽  
Early Type ◽  
Late Type ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
New Ideas ◽  
Integral Field

AbstractWe discuss some recent integral field spectroscopy using the SAURON instrument of a sample consisting of 24 early-type spirals, part of the SAURON Survey, and 18 late-type spirals. Using 2-dimensional maps of their stellar radial velocity, velocity dispersion, and absorption line strength, it is now much easier to understand the nature of nearby galactic bulges. We discuss a few highlights of this work, and point out some new ideas about the formation of galactic bulges.

scholarly journals An Oxford SWIFT integral field spectroscopy study of 14 early-type galaxies in the Coma cluster

2012 ◽  
Vol 425 (2) ◽  
pp. 1521-1526 ◽  
Author(s):  
Nicholas Scott ◽  
Ryan Houghton ◽  
Roger L. Davies ◽  
Michele Cappellari ◽  
Niranjan Thatte ◽  
...  
Keyword(s):  
Spectroscopy Study ◽  
Early Type ◽  
Coma Cluster ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field

scholarly journals Reconstructing the mass assembly history with kinematics and nuclear light profiles

2014 ◽  
Vol 10 (S311) ◽  
pp. 45-48
Author(s):  
Davor Krajnović
Keyword(s):  
Angular Momentum ◽  
Internal Structure ◽  
Early Type ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Mass Assembly ◽  
Light Profiles ◽  
Integral Field

AbstractIn this contribution I show that by combining imaging and integral-field spectroscopy it is possible to unravel the internal structure of galaxies. In particular, I will present the photometric and kinematic evidence for discs linking them with stellar angular momentum content of early-type galaxies. Furthermore, I show that the existence of both fast rotators with core and slow rotators with core-less nuclear light profiles challenges the standard formation scenarios for fast and slow rotators and suggests new pathways of mass assembly.

The DIVING3D Project: Analysis of the nuclear region of Early-type Galaxies

2020 ◽  
Vol 15 (S359) ◽  
pp. 454-456
Author(s):  
T. V. Ricci ◽  
J. E. Steiner ◽  
R. B. Menezes
Keyword(s):  
Emission Lines ◽  
H Ii Regions ◽  
Sample Type ◽  
Early Type ◽  
Integral Field Spectroscopy ◽  
Project Analysis ◽  
Line Region ◽  
Field Unit ◽  
Integral Field

AbstractIn this work, we present preliminary results regarding the nuclear emission lines of a statistically complete sample of 56 early-type galaxies that are part of the Deep Integral Field Spectroscopy View of Nuclei of Galaxies (DIVING3D) Project. All early type galaxies (ETGs) were observed with the Gemini Multi-Object Spectrograph Integral Field Unit (GMOS-IFU) installed on the Gemini South Telescope. We detected emission lines in 93% of the sample, mostly low-ionization nuclear emission-line region galaxies (LINERs). We did not find Transition Objects nor H II regions in the sample. Type 1 objects are seen in ∼23% of the galaxies.

Testing commercial variable fiber attenuators and lenslet arrays for equalized integral field spectroscopy applications

2008 ◽  
Author(s):  
F. Gracia-Temich ◽  
B. García-Lorenzo ◽  
Y. Padilla-Michel ◽  
J. F. M. Escobar-Romero ◽  
J. J. Fuensalida ◽  
...  
Keyword(s):  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field
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