The Effect of Bars on the Ionized ISM: Optical Emission Lines from Milky Way Analogs

Gas interior to the bar of the Milky Way has recently been shown to be the closest example of a low-ionization (nuclear) emission region (LI(N)ER) in the universe. To better understand the nature of this gas, a sample of face-on galaxies with integral field spectroscopy is used to study the ionized...

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Veröffentlicht in:The Astrophysical journal 2020-08, Vol.898 (2), p.116
Hauptverfasser: Krishnarao, Dhanesh, Tremonti, Christy, Fraser-McKelvie, Amelia, Kraljic, Katarina, Boardman, Nicholas Fraser, Masters, Karen L., Benjamin, Robert A., Haffner, L. Matthew, Jones, Amy, Pace, Zachary J., Zasowski, Gail, Bershady, Matthew, Bizyaev, Dmitry, Brinkmann, Jonathan, Brownstein, Joel R., Drory, Niv, Pan, Kaike, Zhang, Kai
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container_issue 2
container_start_page 116
container_title The Astrophysical journal
container_volume 898
creator Krishnarao, Dhanesh
Tremonti, Christy
Fraser-McKelvie, Amelia
Kraljic, Katarina
Boardman, Nicholas Fraser
Masters, Karen L.
Benjamin, Robert A.
Haffner, L. Matthew
Jones, Amy
Pace, Zachary J.
Zasowski, Gail
Bershady, Matthew
Bizyaev, Dmitry
Brinkmann, Jonathan
Brownstein, Joel R.
Drory, Niv
Pan, Kaike
Zhang, Kai
description Gas interior to the bar of the Milky Way has recently been shown to be the closest example of a low-ionization (nuclear) emission region (LI(N)ER) in the universe. To better understand the nature of this gas, a sample of face-on galaxies with integral field spectroscopy is used to study the ionized gas conditions of 240 barred and 250 nonbarred galaxies, focusing on those that are most similar to the Milky Way. Strong optical line emission of [N ii] λ6584, H , [O iii] λ5007, and Hβ are used to diagnose the dominant ionization mechanisms of gas across galaxies and the Galaxy via Baldwin-Phillips-Terlevich diagrams. Barred galaxies show a strong suppression of star formation and an increase in composite and LI(N)ER-like spectra in their inner regions when compared with similar nonbarred counterparts. This effect is lessened in galaxies of very low ( ) or very high ( ) total stellar mass. Bar masks from Galaxy Zoo:3D show the bar's nonaxisymmetric effect on the ionized gas and help predict the face-on distribution of ionized gas conditions near the bar of the Milky Way.
doi_str_mv 10.3847/1538-4357/ab9fa3
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subjects Analogs
ASTRONOMY AND ASTROPHYSICS
Astrophysics
Barred galaxies
Barred spiral galaxies
Emission lines
Galaxies
Integral field spectroscopy
Interstellar atomic gas
Interstellar line emission
Interstellar medium
Interstellar radiation field
Ionization
LINER galaxies
Masks
Milky Way
Milky Way Galaxy
Spectroscopy
Spectrum analysis
Star & galaxy formation
Star formation
Stars
Stars & galaxies
Stellar mass
the Milky Way
title The Effect of Bars on the Ionized ISM: Optical Emission Lines from Milky Way Analogs
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