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19962003
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astro-ph2003

Intergalactic Globular Clusters

Michael J. West, Patrick Cote, Henry C. Ferguson +5

We confirm and extend our previous detection of a population of intergalactic globular clusters in Abell 1185, and report the first discovery of an intergalactic globular cluster i…

astro-ph2002

Using M32 to Study Rapid Phases of Stellar Evolution

Thomas M. Brown, Henry C. Ferguson, Allen V. Sweigart +2

The compact elliptical galaxy M32 offers a unique testing ground for theories of stellar evolution. Because of its proximity, solar-blind UV observations can resolve the hot evolve…

astro-ph1999

Mid-UV Determination of Elliptical Galaxy Abundances and Ages

Jennifer M. Lotz, Henry C. Ferguson, Ralph C. Bohlin

We investigate the effects of abundance and age on the mid-UV spectra and Mg_{2} strengths of stellar populations using simple population synthesis models. These models are used to…

astro-ph1998

An Extremely Red r^{1/4} Galaxy in the Test Image of the Hubble Deep Field South

T. Treu, M. Stiavelli, A. R. Walker +14

We report the serendipitous discovery of an extremely red object in the Hubble Deep Field South (HDFS) Test NICMOS (Near Infrared Camera and Multi Object Spectrograph) field of vie…

astro-ph1998

Globular Clusters in Dwarf Elliptical Galaxies

B. W. Miller, H. C. Ferguson, J. Lotz +2

Globular clusters (GCs) provide one way of determining when the most important periods of star formation in dwarf elliptical (dE) galaxies occurred. Thus, they are also useful for…

astro-ph1996

Far-UV Line Strengths in Elliptical Galaxies

H. C. Ferguson, T. M. Brown, A. F. Davidsen

Much of the far-UV emission from elliptical galaxies is thought to arise from extreme horizontal branch stars and related objects. Only about 10% of the stellar population needs to…