NGC 5011C: an overlooked dwarf galaxy in the Centaurus A group
arXiv:astro-ph/0701280 · doi:10.1086/512157
Abstract
(abridged) We report the discovery of a previously unnoticed member of the Centaurus A Group, NGC 5011C. While the galaxy is a well known stellar system listed with a NGC number its true identity remained hidden because of coordinate confusion and wrong redshifts in the literature. NGC 5011C attracted our attention since, at a putative distance of 45.3 Mpc, it would be a peculiar object having a very low surface brightness typical of a dwarf galaxy, and at the same time having the size of an early-type spiral or S0 galaxy. To confirm or reject this peculiarity, our immediate objective was to have the first reliable measurement of its recession velocity. The observations were carried out with EFOSC2 at the 3.6m ESO telescope. We found that NGC 5011C has indeed a low redshift of v_sun=647+/-96 km/sec and thus is a nearby dwarf galaxy rather than a member of the distant Centaurus cluster as believed for the past 23 years. Rough distance estimates based on photometric parameters also favor this scenario. As a byproduct of our study we update the redshift for NGC 5011B at v_sun=3227+/-50 km/sec. Applying population synthesis techniques, we find that NGC 5011B has a luminosity-weighted age of 4+/-1 Gyr and a solar metallicity, and that the luminosity-weighted age and metallicity of NGC 5011C are 0.9+/-0.1 Gyr and 1/5 solar. Finally we estimate a stellar mass of NGC 5011C comparable to that of dwarf spheroidal galaxies in the Local Group.
13 pages, 6 figures, accepted by the Astronomical Journal
References in corpus (13)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Stellar population synthesis at the resolution of 2003
- The ACS Virgo Cluster Survey. XIII. SBF Distance Catalog and the Three-Dimensional Structure of the Virgo Cluster
- The Local Group and other neighboring galaxy groups
- The Hubble flow around the CenA / M83 galaxy complex
- Discovery of Numerous Dwarf Galaxies in the Two Nearest Groups of Galaxies
- Distances, Metallicities, and Ages of Dwarf Elliptical Galaxies in the Virgo Cluster from Surface Brightness Fluctuations
- Testing the Surface Brightness Fluctuations Method for Dwarf Elliptical Galaxies in the Centaurus A Group
- Spectral Classification of Galaxies Along the Hubble Sequence
- The distance to Hydra and Centaurus from surface brightness fluctuations: Consequences for the Great Attractor model
- Interstellar medium disruption in the Centaurus A group
- HI Detection in two Dwarf S0 Galaxies in Nearby Groups: ESO384-016 and NGC 59
- The star formation history of the LSB Galaxy UGC 5889
Cited by in corpus (8)
- A whirling plane of satellite galaxies around Centaurus A challenges cold dark matter cosmology
- The Local Volume HI Survey (LVHIS)
- New low surface brightness dwarf galaxies in the Centaurus group
- The coherent motion of Cen A dwarf satellite galaxies remains a challenge for CDM cosmology
- Dual Stellar Halos in the Standard Elliptical Galaxy M105 and Formation of Massive Early-Type Galaxies
- The Strikingly Metal-Rich Halo of the Sombrero Galaxy
- Nuclear Water Maser Emission in Centaurus A
- The Cen A galaxy group: dynamical mass and missing baryons