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Investigating the evolution of merger remnants from the formation of gas disks

by Wilner, David J. , Kawabe, Ryohei , Crocker, Alison F. , Kaneko, Hiroyuki , Ueda, Junko , Hatsukade, Bunyo , Tamura, Yoichi , Iono, Daisuke , Yun, Min S. , Komugi, Shinya , Pan, Hsi-An , Matsuda, Yuichi , Narayanan, Desika , Espada, Daniel

in Astronomical bodies / Astronomy / Astrophysics / Carbon monoxide / Contributed Papers / Formations / Galactic disk / Galactic evolution / Galaxies / Gases / Interferometry / Kinematics / Star & galaxy formation

2014

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Investigating the evolution of merger remnants from the formation of gas disks

2014

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2014

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Journal Article

Investigating the evolution of merger remnants from the formation of gas disks

Wilner, David J.,

Kawabe, Ryohei,

Crocker, Alison F.,

Kaneko, Hiroyuki,

Ueda, Junko,

Hatsukade, Bunyo,

Tamura, Yoichi,

Iono, Daisuke,

Yun, Min S.,

Komugi, Shinya,

Pan, Hsi-An,

Matsuda, Yuichi,

Narayanan, Desika,

Espada, Daniel

2014

Overview

Our new compilation of interferometric CO data suggests that nuclear and extended molecular gas disks are common in the final stages of mergers. Comparing the sizes of the molecular gas disk and gas mass fractions to early-type and late-type galaxies, about half of the sample show similar properties to early-type galaxies, which have compact gas disks and low gas mass fractions. We also find that sources with extended gas disks and large gas mass fractions may become disk-dominated galaxies.

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Cambridge University Press

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