Galaxy formation and mergers with stars and massive black holes

Placeholder Show Content

Abstract/Contents

Abstract
While mounting observational evidence suggests the coevolution of galaxies and their embedded massive black holes (MBHs), a comprehensive astrophysical understanding which incorporates both galaxies and MBHs has been missing. To tackle the nonlinear processes of galaxy formation, we develop a state-of-the-art numerical framework which self-consistently models the interplay between galactic components: dark matter, gas, stars, and MBHs. Utilizing this physically motivated tool, we present an investigation of a massive star-forming galaxy hosting a slowly growing MBH in a cosmological LCDM simulation. The MBH feedback heats the surrounding gas and locally suppresses star formation in the galactic inner core. In simulations of merging galaxies, the high-resolution adaptive mesh allows us to observe widespread starbursts via shock-induced star formation, and the interplay between the galaxies and their embedding medium. Fast growing MBHs in merging galaxies drive more frequent and powerful jets creating sizable bubbles at the galactic centers. We conclude that the interaction between the interstellar gas, stars and MBHs is critical in understanding the star formation history, black hole accretion history, and cosmological evolution of galaxies. Expanding upon our extensive experience in galactic simulations, we are well poised to apply this tool to other challenging, yet highly rewarding tasks in contemporary astrophysics, such as high-redshift quasar formation.

Description

Type of resource text
Form electronic; electronic resource; remote
Extent 1 online resource.
Publication date 2011
Issuance monographic
Language English

Creators/Contributors

Associated with Kim, Chi-hun
Associated with Stanford University, Department of Physics
Primary advisor Abel, Tom G, 1970-
Thesis advisor Abel, Tom G, 1970-
Thesis advisor Allen, Steven G
Thesis advisor Wechsler, Risa H. (Risa Heyrman)
Advisor Allen, Steven G
Advisor Wechsler, Risa H. (Risa Heyrman)

Subjects

Genre Theses

Bibliographic information

Statement of responsibility Ji-hoon Kim.
Note Submitted to the Department of Physics.
Thesis Ph.D. Stanford University 2011
Location electronic resource

Access conditions

Copyright
© 2011 by Ji-hoon Kim

Also listed in

Loading usage metrics...