2011ApJ...734...87R


Query : 2011ApJ...734...87R

2011ApJ...734...87R - Astrophys. J., 734, 87 (2011/June-3)

Galaxy-wide shocks in late-merger stage luminous infrared galaxies.

RICH J.A., KEWLEY L.J. and DOPITA M.A.

Abstract (from CDS):

We present an integral field spectroscopic study of two nearby luminous infrared galaxies (LIRGs), IC 1623 and NGC 3256, which exhibit evidence of widespread shock excitation induced by ongoing merger activity. We show the importance of carefully separating excitation due to shocks versus excitation by H II regions and the usefulness of integral field unit data in interpreting the complex processes in LIRGs. Our analysis focuses primarily on the emission line gas, which is extensive in both systems and is a result of the abundant ongoing star formation as well as widespread LINER-like excitation from shocks. We use emission line ratio maps, line kinematics, line-ratio diagnostics, and new models as methods for distinguishing and analyzing shocked gas in these systems. We discuss how our results inform the merger sequence associated with local U/LIRGs and the impact that widespread shock excitation has on the interpretation of emission line spectra and derived quantities of both local and high-redshift galaxies.

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Journal keyword(s): galaxies: evolution - galaxies: individual (NGC 3256, IC 1623) - galaxies: ISM - shock waves

Simbad objects: 7

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Number of rows : 7
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 IC 1623A EmG 01 07 46.57800 -17 30 22.2192   14.34   12.71   ~ 66 1
2 IC 1623 IG 01 07 47.24 -17 30 25.0   15       ~ 338 2
3 IC 1623B Sy1 01 07 47.569 -17 30 25.04   15.04   14.07   ~ 78 1
4 NGC 839 EmG 02 09 42.73127 -10 11 01.6370   13.98 11.42 12.70   ~ 161 1
5 LAWD 25 WD* 07 40 20.7886676070 -17 24 49.156867583   13.36 13.061 12.886 12.70 DZQA6 218 0
6 NGC 3256 Sy2 10 27 51.284 -43 54 13.55   11.83 11.33 10.62 11.9 ~ 920 2
7 LAWD 74 WD* 19 20 34.9229289504 -07 40 00.065957592 11.553 12.345 12.290 12.229 12.164 DBQA5 250 0

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