Volume 506, Number 2, November I 2009
|Page(s)||677 - 680|
|Published online||03 September 2009|
HI-observations of dwarf galaxies in the Local Supercluster*
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany e-mail: email@example.com
2 Special Astrophysical Institute, Russian Academy of Sciences, N. Arkhyz, KChR, 369167, Russia e-mail: firstname.lastname@example.org
3 Astronomical Observatory of Kiev University, Kiev, Ukraine e-mail: email@example.com
Accepted: 29 June 2009
We have observed 71 dwarf galaxies of low surface brightness using the 100-m radio telescope at Effelsberg in a search for new members of 27 northern galaxy groups with characteristic distances of 8 to 15 Mpc. We present radial velocities, HI-fluxes, and HI line widths for 17 detected galaxies as well as upper limits for the remaining undetected objects. Almost all detected dwarf galaxies are physical members of the corresponding group with a mean radial velocity difference of -9 ± 45 km s-1 with respect to the principal galaxy in each group. Our sample of new dwarf members of nearby groups has a median radial velocity of 700 km s-1, a mean blue absolute magnitude of –12.7 mag, a mean linear diameter of 2.5 kpc, and a mean MHI/LB ratio of 1.1 /. The Ir galaxy d1217+4703 in the Canes Venatici I cloud turns out to be a very gas-rich galaxy with MHI/LB = 6.5 in solar units.
Key words: galaxies: dwarf / galaxies: evolution / galaxies: ISM
© ESO, 2009
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.