Internal Dynamics, Structure, and Formation of Dwarf Elliptical Galaxies. I. A Keck/[ITAL]Hubble Space Telescope[/ITAL] Study of Six Virgo Cluster Dwarf Galaxies

2002 ◽  
Vol 124 (6) ◽  
pp. 3073-3087 ◽  
Author(s):  
M. Geha ◽  
P. Guhathakurta ◽  
R. P. van der Marel
1994 ◽  
Vol 108 ◽  
pp. 1598 ◽  
Author(s):  
L. Ferrarese ◽  
F. C. van den Bosch ◽  
H. C. Ford ◽  
W. Jaffe ◽  
R. W. O'Connell

1994 ◽  
Vol 108 ◽  
pp. 1579 ◽  
Author(s):  
Frank C. van den Bosch ◽  
Laura Ferrarese ◽  
Walter Jaffe ◽  
Holland C. Ford ◽  
Robert W. O'Connell

1994 ◽  
Vol 108 ◽  
pp. 1567 ◽  
Author(s):  
W. Jaffe ◽  
H. C. Ford ◽  
R. W. O'Connell ◽  
F. C. van den Bosch ◽  
L. Ferrarese

2007 ◽  
Vol 3 (S248) ◽  
pp. 244-247 ◽  
Author(s):  
S. Piatek ◽  
C. Pryor

AbstractOver the past several years, our research group has been measuring proper motions for nearby dwarf satellite galaxies using data taken with the Hubble Space Telescope. In order to measure proper motions with an expected size of several tens of milliarcseconds per century using a time baseline of 2-4 years, our work required that positions of stars and QSOs be measured to an accuracy of ~0.25 mas (~0.005 pixel). This contribution reviews the scientific justification of this work and our methodology. It concludes with a few general results and future directions.


1986 ◽  
Vol 92 ◽  
pp. 1007 ◽  
Author(s):  
Gregory D. Bothun ◽  
Jeremy R. Mould ◽  
Nelson Caldwell ◽  
Harvey T. MacGillivray

2001 ◽  
Vol 205 ◽  
pp. 154-161 ◽  
Author(s):  
Roeland P. van der Marel

This review summarizes some aspects of the central kiloparsec scale structure of galaxies, and in particular spiral galaxies, elliptical galaxies and merger remnants. The focus is on results from optical and near-IR imaging and spectroscopy, with emphasis on recent work with the Hubble Space Telescope.


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