Volume 391, Number 1, August III 2002
|Page(s)||103 - 115|
|Section||Cosmology (including clusters of galaxies)|
|Published online||29 July 2002|
Near-Infrared photometry in the J, H and bands for Polar Ring Galaxies
I. Data, structural parameters
INAF – Osservatorio Astronomico di Capodimonte (OAC), via Moiariello 16, 80131 Napoli, Italy
2 International School for Advanced Studied (ISAS), via Beirut 2-4, 34014 Trieste, Italy
3 University of Wisconsin, Department of Astronomy, 475 N. Charter St., Madison, WI, USA
4 RSAA, Mt. Stromlo, Canberra, Cotter Road, Weston ACT 2611, Australia
Corresponding author: E. Iodice, email@example.com
Accepted: 15 May 2002
We present new Near-Infrared (NIR) observations, in the J, H and Kn bands, for a sample of Polar Ring Galaxies (PRGs), selected from the Polar Ring Catalogue (Whitmore et al. [CITE]). Data were acquired with the CASPIR near-IR camera at the 2.3 m telescope of Mount Stromlo and Siding Spring Observatory. We report here on the detail morphological study for the central host galaxy and the polar structure in all PRGs of our sample. Total magnitudes, bulge-to-disk decomposition and structural parameters are computed for all objects. These data are crucial for an accurate modeling of the stellar population and the estimate of the star formation rates in the two components.
Key words: galaxies: peculiar / galaxies: photometry / galaxies: fundamental parameters
© ESO, 2002
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.