Open Access. Powered by Scholars. Published by Universities.®

Physical Sciences and Mathematics Commons

Open Access. Powered by Scholars. Published by Universities.®

Astrophysics and Astronomy

PDF

University of Massachusetts Amherst

Open Access Dissertations

Theses/Dissertations

Galaxies

Articles 1 - 2 of 2

Full-Text Articles in Physical Sciences and Mathematics

The Aztec Millimeter-Wave Camera: Design, Integration, Performance, And The Characterization Of The (Sub-)Millimeter Galaxy Population, Jason Edward Austermann May 2009

The Aztec Millimeter-Wave Camera: Design, Integration, Performance, And The Characterization Of The (Sub-)Millimeter Galaxy Population, Jason Edward Austermann

Open Access Dissertations

One of the primary drivers in the development of large format millimeter detector arrays is the study of sub-millimeter galaxies (SMGs) - a population of very luminous high-redshift dust-obscured starbursts that are widely believed to be the dominant contributor to the Far-Infrared Background (FIB). The characterization of such a population requires the ability to map large patches of the (sub-)millimeter sky to high sensitivity within a feasible amount of time. I present this dissertation on the design, integration, and characterization of the 144-pixel AzTEC millimeter-wave camera and its application to the study of the sub-millimeter galaxy population. In particular, I …


The Role Of Stellar Feedback In Galaxy Evolution, Li Zhiyuan Feb 2009

The Role Of Stellar Feedback In Galaxy Evolution, Li Zhiyuan

Open Access Dissertations

Aiming at understanding the role of stellar feedback in galaxy evolution, I present a study of the hot interstellar medium in several representative galaxies, based primarily on X-ray observations as well as theoretical modelling. I find that, in the massive disk galaxies NGC2613 and M104, the observed amount of hot gas is much less than that predicted by current galaxy formation models. Such a discrepancy suggests a lack of appropriate treatments of stellar/AGN feedback in these models. I also find that stellar feedback, primarily in the form of mass loss from evolved stars and energy released from supernovae, and presumably …