TY - CHAP
T1 - Characterizing barred galaxies in the Abell 901/902 Supercluster from STAGES
AU - Marinova, Irina
AU - Jogee, Shardha
AU - Bacon, David
AU - Balogh, Michael L.
AU - Barden, Marco
AU - Barazza, Fabio D.
AU - Bell, Eric F.
AU - Bohm, Asmus
AU - Caldwell, John A. R.
AU - Gray, Meghan E.
AU - Haussler, Boris
AU - Heymans, Catherine
AU - Jahnke, Knud
AU - Van Kampen, Eelco
AU - Koposov, S.
AU - Lane, Kyle
AU - McIntosh, Daniel H.
AU - Meisenheimer, Klaus
AU - Peng, Chien Y.
AU - Rix, Hans-Walter
AU - Sanchez, Sebastian F.
AU - Taylor, Andy
AU - Wisotzki, Lutz
AU - Wolf, Christian
AU - Zheng, X.
PY - 2008
Y1 - 2008
N2 - In dense clusters, higher densities at early epochs as well as physical processes, such as ram pressure stripping and tidal interactions become important, and can have direct consequences for the evolution of bars and their host disks. To study bars and disks as a function of environment, we are using the STAGES ACS HST survey of the Abell 901/902 supercluster (z~0.165), along with earlier field studies based the SDSS and the Ohio State University Bright Spiral Galaxy Survey (OSUBSGS). We explore the limitations of traditional methods for characterizing the bar fraction, and in particular highlight uncertainties in disk galaxy selection in cluster environments. We present an alternative approach for exploring the proportion of bars, and investigate the properties of bars as a function of host galaxy color, Sersic index, stellar mass, star formation rate (SFR), specific SFR, and morphology.
AB - In dense clusters, higher densities at early epochs as well as physical processes, such as ram pressure stripping and tidal interactions become important, and can have direct consequences for the evolution of bars and their host disks. To study bars and disks as a function of environment, we are using the STAGES ACS HST survey of the Abell 901/902 supercluster (z~0.165), along with earlier field studies based the SDSS and the Ohio State University Bright Spiral Galaxy Survey (OSUBSGS). We explore the limitations of traditional methods for characterizing the bar fraction, and in particular highlight uncertainties in disk galaxy selection in cluster environments. We present an alternative approach for exploring the proportion of bars, and investigate the properties of bars as a function of host galaxy color, Sersic index, stellar mass, star formation rate (SFR), specific SFR, and morphology.
M3 - Chapter (peer-reviewed)
SN - 9781583816561
T3 - Astronomical Society of the Pacific conference series
SP - 231
EP - 234
BT - New horizons in astronomy
PB - Astronomical Society of the Pacific
CY - Orem
T2 - Frank N. Bash Symposium 2007
Y2 - 1 January 2008
ER -