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EnglishRecent observations with the Australia Telescope Compact Array show that the elliptical galaxy NGC 5266 has a disk of neutral hydrogen extending to almost 10Re. This HI disk lies along the galaxy's major axis, at right angles to the inner minor-axis dust lane. The geometry and kinematics of the gas will allow us to determine both the intrinsic shape of the stellar galaxy and the mass distribution. The mass-to-light ratio M/L_B rises from about 2 in the central regions to ~12 at 9Re (H0=50 km/s/Mpc).
| Titolo: | HI in the Dusty Elliptical Galaxy NGC5266 | |
| Autori: | ||
| Data di pubblicazione: | 1995 | |
| Rivista: | ||
| Abstract: | Recent observations with the Australia Telescope Compact Array show that the elliptical galaxy NGC 5266 has a disk of neutral hydrogen extending to almost 10Re. This HI disk lies along the galaxy's major axis, at right angles to the inner minor-axis dust lane. The geometry and kinematics of the gas will allow us to determine both the intrinsic shape of the stellar galaxy and the mass distribution. The mass-to-light ratio M/L_B rises from about 2 in the central regions to ~12 at 9Re (H0=50 km/s/Mpc). | |
| Handle: | http://hdl.handle.net/11577/142996 | |
| Appare nelle tipologie: | 01.01 - Articolo in rivista |
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