Eight billion years of disk galaxy evolution no galaxy is an island

GEMS, MIPS Instrument, and COMBO-17 teams

doi:10.1007/978-1-4020-5573-7_82

Eight billion years of disk galaxy evolution no galaxy is an island

GEMS, MIPS Instrument, and COMBO-17 teams

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

We present a brief discussion of the evolution of disk galaxy stellar masses, sizes, rotation velocities, and star formation rates over the last eight billion years. Recent observations have failed to detect significant evolution in the stellar mass Tully-Fisher relation, stellar mass–size relation, and the stellar mass function of disk galaxies. Yet, most z < 1 star formation is in disks, and this star formation would be expected to drive a rapid growth of the total stellar mass (and therefore mass function) of disks in the last eight billion years. Such a build-up is not seen; instead, a rapid build-up in the total stellar mass in non-star-forming spheroid-dominated galaxies is observed. Large numbers of disk-dominated galaxies are systematically shutting off their star formation and building up a spheroid (or losing a disk) in the epoch 0 < z < 1.

Original language	English (US)
Title of host publication	Astrophysics and Space Science Proceedings
Editors	R.S. De Jong
Publisher	Springer Science and Business Media B.V.
Pages	475-480
Number of pages	6
ISBN (Electronic)	9781402055737
ISBN (Print)	9780387727677, 9780387876207, 9781402055720, 9781402055720, 9781402069321, 9781402088674, 9781402091896, 9781441981608, 9781441983688, 9783540758259, 9783642033230, 9783642103216, 9783642103513, 9783642113406, 9783642172502, 9789048133994, 9789048134984
DOIs	https://doi.org/10.1007/978-1-4020-5573-7_82
State	Published - 2007
Event	International Conference on Island Universe: Structure and Evolution of Disk Galaxies, 2005 - Terschelling, Netherlands Duration: Jul 3 2005 → Jul 5 2005

Publication series

Name	Astrophysics and Space Science Proceedings
Volume	0
ISSN (Print)	1570-6591
ISSN (Electronic)	1570-6605

Conference

Conference	International Conference on Island Universe: Structure and Evolution of Disk Galaxies, 2005
Country/Territory	Netherlands
City	Terschelling
Period	7/3/05 → 7/5/05

Keywords

Galaxies: Evolution
Galaxies: Fundamental parameters
Infrared: Galaxies

ASJC Scopus subject areas

General Physics and Astronomy
Computer Science Applications
Spectroscopy
Space and Planetary Science
Nuclear and High Energy Physics

Access to Document

10.1007/978-1-4020-5573-7_82

Cite this

Eight billion years of disk galaxy evolution no galaxy is an island. / GEMS, MIPS Instrument, and COMBO-17 teams.
Astrophysics and Space Science Proceedings. ed. / R.S. De Jong. Springer Science and Business Media B.V., 2007. p. 475-480 (Astrophysics and Space Science Proceedings; Vol. 0).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

GEMS, MIPS Instrument, and COMBO-17 teams 2007, Eight billion years of disk galaxy evolution no galaxy is an island. in RS De Jong (ed.), Astrophysics and Space Science Proceedings. Astrophysics and Space Science Proceedings, vol. 0, Springer Science and Business Media B.V., pp. 475-480, International Conference on Island Universe: Structure and Evolution of Disk Galaxies, 2005, Terschelling, Netherlands, 7/3/05. https://doi.org/10.1007/978-1-4020-5573-7_82

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title = "Eight billion years of disk galaxy evolution no galaxy is an island",

abstract = "We present a brief discussion of the evolution of disk galaxy stellar masses, sizes, rotation velocities, and star formation rates over the last eight billion years. Recent observations have failed to detect significant evolution in the stellar mass Tully-Fisher relation, stellar mass–size relation, and the stellar mass function of disk galaxies. Yet, most z < 1 star formation is in disks, and this star formation would be expected to drive a rapid growth of the total stellar mass (and therefore mass function) of disks in the last eight billion years. Such a build-up is not seen; instead, a rapid build-up in the total stellar mass in non-star-forming spheroid-dominated galaxies is observed. Large numbers of disk-dominated galaxies are systematically shutting off their star formation and building up a spheroid (or losing a disk) in the epoch 0 < z < 1.",

keywords = "Galaxies: Evolution, Galaxies: Fundamental parameters, Infrared: Galaxies",

author = "{GEMS, MIPS Instrument, and COMBO-17 teams} and Bell, {Eric F.} and Marco Barden and Xianzhong Zheng and Casey Papovich and {Le Floc{\textquoteright}H}, Emeric and George Rieke and Christian Wolf",

note = "Publisher Copyright: {\textcopyright} 2007, Springer Netherlands. All rights reserved.; International Conference on Island Universe: Structure and Evolution of Disk Galaxies, 2005 ; Conference date: 03-07-2005 Through 05-07-2005",

year = "2007",

doi = "10.1007/978-1-4020-5573-7_82",

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AU - GEMS, MIPS Instrument, and COMBO-17 teams

AU - Bell, Eric F.

AU - Barden, Marco

AU - Zheng, Xianzhong

AU - Papovich, Casey

AU - Le Floc’H, Emeric

AU - Rieke, George

AU - Wolf, Christian

PY - 2007

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N2 - We present a brief discussion of the evolution of disk galaxy stellar masses, sizes, rotation velocities, and star formation rates over the last eight billion years. Recent observations have failed to detect significant evolution in the stellar mass Tully-Fisher relation, stellar mass–size relation, and the stellar mass function of disk galaxies. Yet, most z < 1 star formation is in disks, and this star formation would be expected to drive a rapid growth of the total stellar mass (and therefore mass function) of disks in the last eight billion years. Such a build-up is not seen; instead, a rapid build-up in the total stellar mass in non-star-forming spheroid-dominated galaxies is observed. Large numbers of disk-dominated galaxies are systematically shutting off their star formation and building up a spheroid (or losing a disk) in the epoch 0 < z < 1.

AB - We present a brief discussion of the evolution of disk galaxy stellar masses, sizes, rotation velocities, and star formation rates over the last eight billion years. Recent observations have failed to detect significant evolution in the stellar mass Tully-Fisher relation, stellar mass–size relation, and the stellar mass function of disk galaxies. Yet, most z < 1 star formation is in disks, and this star formation would be expected to drive a rapid growth of the total stellar mass (and therefore mass function) of disks in the last eight billion years. Such a build-up is not seen; instead, a rapid build-up in the total stellar mass in non-star-forming spheroid-dominated galaxies is observed. Large numbers of disk-dominated galaxies are systematically shutting off their star formation and building up a spheroid (or losing a disk) in the epoch 0 < z < 1.

KW - Galaxies: Evolution

KW - Galaxies: Fundamental parameters

KW - Infrared: Galaxies

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ER -

Eight billion years of disk galaxy evolution no galaxy is an island

Abstract

Publication series

Conference

Keywords

ASJC Scopus subject areas

Access to Document

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