A subsample of six objects, which have the most disk-like gas distribution, was selected for long-slit spectroscopy at the ESO 3.6-m and ESO/MPI 2.2-m telescopes in order to map the gas velocity field. The photometric and kinematic results were then used to constrain the intrinsic shape and mass distribution of the host galaxy.
The distribution of ionised gas in early-type galaxies.
BERTOLA, FRANCESCO;PIZZELLA, ALESSANDRO;SAGLIA, ROBERTO PHILIP;
1996
Abstract
A subsample of six objects, which have the most disk-like gas distribution, was selected for long-slit spectroscopy at the ESO 3.6-m and ESO/MPI 2.2-m telescopes in order to map the gas velocity field. The photometric and kinematic results were then used to constrain the intrinsic shape and mass distribution of the host galaxy.File in questo prodotto:
Non ci sono file associati a questo prodotto.
Pubblicazioni consigliate
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
