scholarly journals From star-forming spirals to passive spheroids: integral field spectroscopy of E+A galaxies

2011 ◽  
Vol 420 (1) ◽  
pp. 672-683 ◽  
Author(s):  
A. M. Swinbank ◽  
M. L. Balogh ◽  
R. G. Bower ◽  
A. I. Zabludoff ◽  
J. R. Lucey ◽  
...  
Keyword(s):  
Star Forming ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field

scholarly journals Integral Field Spectroscopy of High‐Redshift Star‐forming Galaxies with Laser‐guided Adaptive Optics: Evidence for Dispersion‐dominated Kinematics

2007 ◽  
Vol 669 (2) ◽  
pp. 929-946 ◽  
Author(s):  
David R. Law ◽  
Charles C. Steidel ◽  
Dawn K. Erb ◽  
James E. Larkin ◽  
Max Pettini ◽  
...  
Keyword(s):  
Adaptive Optics ◽  
High Redshift ◽  
Star Forming ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field

scholarly journals THE SINS SURVEY: SINFONI INTEGRAL FIELD SPECTROSCOPY OFz∼ 2 STAR-FORMING GALAXIES

2009 ◽  
Vol 706 (2) ◽  
pp. 1364-1428 ◽  
Author(s):  
N. M. Förster Schreiber ◽  
R. Genzel ◽  
N. Bouché ◽  
G. Cresci ◽  
R. Davies ◽  
...  
Keyword(s):  
Star Forming ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field

scholarly journals Mapping the Dynamics of the Quasar 3C 48

2001 ◽  
Vol 205 ◽  
pp. 162-165
Author(s):  
Eleni T. Chatzichristou
Keyword(s):  
Emission Line ◽  
Radio Source ◽  
Star Forming ◽  
Physical Conditions ◽  
Star Forming Regions ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Ir Emission ◽  
Integral Field ◽  
Extended Emission

The archetypical, nearby (z=0.37) quasar 3C 48 is an unusual CSS radio source with excess far-IR emission, whose one-sided radio jet is aligned with the extended ionized emission and a putative second nucleus. Because of its high AGN luminosity and proximity, 3C 48 is a good candidate to search for kinematic signatures of the radio jet-gas coupling and/or of a recent interaction. The radio morphology and our ground-based integral field spectroscopy suggest that the jet is interacting with its immediate environment. Using STIS aboard HST in several slit positions within the central 1”, we map the kinematics and physical conditions of the extended emission line gas and their relations to near-nuclear star forming regions found in existing HST images.

IRX–βRELATION OF STAR-FORMING REGIONS IN NGC 628 BASED ON INTEGRAL FIELD SPECTROSCOPY

2016 ◽  
Vol 826 (2) ◽  
pp. 209 ◽  
Author(s):  
Chengyun Ye ◽  
Hu Zou ◽  
Lin Lin ◽  
Jianhui Lian ◽  
Ning Hu ◽  
...  
Keyword(s):  
Star Forming ◽  
Star Forming Regions ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field

scholarly journals Near‐Infrared Integral Field Spectroscopy of Star‐forming Galaxies

2004 ◽  
Vol 601 (2) ◽  
pp. 813-830 ◽  
Author(s):  
Daniel A. Dale ◽  
Helene Roussel ◽  
Alessandra Contursi ◽  
George Helou ◽  
Harriet L. Dinerstein ◽  
...  
Keyword(s):  
Near Infrared ◽  
Star Forming ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field

scholarly journals Integral field spectroscopy of local LCBGs: NGC 7673, a case study. Physical properties of star-forming regions

2010 ◽  
Vol 411 (3) ◽  
pp. 1819-1832 ◽  
Author(s):  
A. Castillo-Morales ◽  
J. Gallego ◽  
J. Pérez-Gallego ◽  
R. Guzmán ◽  
J. C. Muñoz-Mateos ◽  
...  
Keyword(s):  
Physical Properties ◽  
Star Forming ◽  
Star Forming Regions ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field

scholarly journals Emission-Line Diagnostics for Galaxies

2015 ◽  
Vol 11 (A29B) ◽  
pp. 264-264
Author(s):  
Lisa J. Kewley
Keyword(s):  
Star Formation ◽  
Emission Line ◽  
Power Sources ◽  
Star Forming ◽  
Spatially Resolved ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Yield Information ◽  
Ir Diagnostics ◽  
Integral Field

AbstractI will give an overview of the emission-line diagnostics used for star-forming galaxies. I will review the UV, optical, and IR diagnostics that can be used to yield information about the ISM conditions, star-formation properties, and power sources in GRB hosts, both globally, and with spatially-resolved data. I will discuss wide integral field spectroscopy and AO-led integral field spectroscopy on current and future telescopes, focusing on the insights to be gained on the properties of GRB sites.

scholarly journals Ionized gas outflows and global kinematics of low-z luminous star-forming galaxies

2014 ◽  
Vol 10 (S309) ◽  
pp. 73-76
Author(s):  
S. Arribas ◽  
L. Colina ◽  
E. Bellocchi ◽  
R. Maiolino ◽  
M. Villar-Martín
Keyword(s):  
Interstellar Medium ◽  
Representative Sample ◽  
High Signal ◽  
Signal To Noise ◽  
Ionized Gas ◽  
Star Forming ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Integral Field ◽  
Kinematic Properties

AbstractWe have studied the kinematic properties of the ionized gas outflows and ambient interstellar medium (ISM) in a large and representative sample of local U/LIRGs (58 systems, 75 galaxies) at galactic and sub-galactic (i.e.,star-forming clumps) scales, thanks to integral field spectroscopy (IFS)-based high signal-to-noise integrated spectra. The main results have been recently presented in Arribas et al. (2014), and are briefly summarized here.

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.

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