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:
| File | Dimensione | Formato | |
|---|---|---|---|
|
1996_Msngr_85_30_Zeilinger_KeyProg.pdf
embargo fino al 31/12/2026
Tipologia:
Published (publisher's version)
Licenza:
Accesso gratuito
Dimensione
868.74 kB
Formato
Adobe PDF
|
868.74 kB | Adobe PDF | Visualizza/Apri Richiedi una copia |
Pubblicazioni consigliate
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
