A peculiar object in M51: fuzzy star cluster or a background galaxy?
arXiv:0711.0722 · doi:10.1051/0004-6361:20078359
Abstract
Aims: We study a peculiar object with a projected position close to the nucleus of M51. It is unusually large for a star cluster in M51 and we therefore investigate the three most likely options to explain this object: (a) a background galaxy, (b) a cluster in the disk of M51 and (c) a cluster in M51, but in front of the disk. Methods: We use HST/ACS and HST/NICMOS broad-band photometry to study the properties of this object. Assuming the object is a star cluster, we fit the metallicity, age, mass and extinction using simple stellar population models. Assuming the object is a background galaxy, we estimate the extinction from the colour of the background around the object. We study the structural parameters of the object by fitting the spatial profile with analytical models. Results: We find de-reddened colours of the object which are bluer than expected for a typical elliptical galaxy, and the central surface brightness is brighter than the typical surface brightness of a disc galaxy. It is therefore not likely that the object is a background galaxy. Assuming the object is a star cluster in the disc of M51, we estimate an age and mass of 0.7 Gyr and 2.2 x 10^5 \msun, respectively (with the extinction fixed to E(B-V) = 0.2). Considering the large size of the object, we argue that in this scenario we observe the cluster just prior to final dissolution. If we fit for the extinction as a free parameter, a younger age is allowed and the object is not close to final dissolution. Alternatively, the object could be a star cluster in M51, but in front of the disc, with an age of 1.4 Gyr and mass M = 1.7 x 10^5 \msun. Its effective radius is between ~12-25 pc. This makes the object a "fuzzy star cluster", raising the issue of how an object of this age would end up outside the disc.
arXiv comment7 pages, 5 figures. Journal-ref and DOI added. 2 typos corrected. Added corrections to proof including 1 reference
References in corpus (23)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances
- Dynamical evolution of star clusters in tidal fields
- Spectral and Photometric Evolution of Young Stellar Populations: the Impact of Gaseous Emission at Various Metallicities
- Young massive star clusters in nearby galaxies. II.Software tools, data reductions and cluster sizes
- An analytical description of the disruption of star clusters in tidal fields with an application to Galactic open clusters
- Star cluster disruption by giant molecular clouds
- The ACS Virgo Cluster Survey X. Half-light Radii of Globular Clusters in Early-Type Galaxies: Environmental Dependencies and a Standard Ruler for Distance Estimation
- GEMS: The Size Evolution of Disk Galaxies
- Planetary Nebulae as standard candles XI. Application to Spiral Galaxies
- The Structure and Environment of Young Stellar Clusters in Spiral Galaxies
- The Star Cluster Population of M51: II. Age distribution and relations among the derived parameters
- Star Cluster Formation and Disruption Time-Scales -- I. An empirical determination of the disruption time of star clusters in four galaxies
- Analysing observed star cluster SEDs with evolutionary synthesis models: Systematic uncertainties
- HST observations of star clusters in NGC 1023: Evidence for three cluster populations?
- The effect of spiral arm passages on the evolution of stellar clusters
- The Star Cluster Population of M51: III. Cluster disruption and formation history
- ACS imaging of star clusters in M51. I. Identification and radius distribution
- The Opacity of Spiral Galaxy Disks IV: Radial Extinction Profiles from Counts of Distant Galaxies seen through Foreground Disks
- Multiaperture Photometry of Galaxies in the Coma Cluster
- Chemically consistent evolution of galaxies: II. Spectrophotometric evolution from zero to high redshift
- The Infrared Surface Brightness Fluctuation Distances to the Hydra and Coma Clusters
- UV Colors and Extinctions of HII Regions in the Whirlpool Galaxy (M51)