Spatially resolved kinematics, galactic wind, and quenching of star formation in the luminous infrared galaxy IRAS F11506-3851

Spatially resolved kinematics, galactic wind, and quenching of star formation in the luminous infrared galaxy IRAS F11506-3851

We present a multi-wavelength integral field spectroscopic (IFS) study of the low-z luminous infrared galaxy IRAS F11506-3851 (ESO 320-G030) on the basis of the moderate spectral resolution observations (R ~ 3400−4000) taken with the VIMOS and SINFONI instruments at the ESO VLT. The morphology and t...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2014-09, Vol.569, p.1-14
Hauptverfasser: Cazzoli, S., Arribas, S., Colina, L., Piqueras-López, J., Bellocchi, E., Emonts, B., Maiolino, R.
Format: Artikel
Sprache:eng
Schlagworte:
Astronomy
Galactic winds
galaxies: starburst
Infrared
Interstellar matter
ISM: jets and outflows
ISM: kinematics and dynamics
Kinematics
Quenching
Spectral resolution
Star formation
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Zusammenfassung:We present a multi-wavelength integral field spectroscopic (IFS) study of the low-z luminous infrared galaxy IRAS F11506-3851 (ESO 320-G030) on the basis of the moderate spectral resolution observations (R ~ 3400−4000) taken with the VIMOS and SINFONI instruments at the ESO VLT. The morphology and the 2D kinematics of the gaseous (neutral and ionized) and stellar components have been mapped in the central regions (
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/201323296